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Cassini >> MIMI

CASSINI SATURN MIMI LEMMS CALIBRATED DATA ARCHIVE
CO-S-MIMI-4-LEMMS-CALIB-V1.0	PDS 3 CERTIFIED

Start Time: 2004-01-01 08:00:00 - Stop Time: 2017-09-16 10:00:00

CASSINI SATURN MIMI LEMMS CALIBRATED DATA ARCHIVE

Citiation Information

Author	Vandegriff J., Kusterer M.B.
Title	CASSINI SATURN MIMI LEMMS CALIBRATED DATA ARCHIVE
Publisher	NASA Planetary Data System
Publication Year	2018
doi	https://doi.org/10.17189/1519608

Top/ DATA/ LPHAAVG0_1MIN/ 2004 /

LPHAAVG0_1MIN_2004001_01

Start Time:	2004-001T00:00	Stop Time:	2004-002T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004002_01

Start Time:	2004-002T00:00	Stop Time:	2004-003T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004003_01

Start Time:	2004-003T00:00	Stop Time:	2004-004T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004004_01

Start Time:	2004-004T00:00	Stop Time:	2004-005T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004005_01

Start Time:	2004-005T00:00	Stop Time:	2004-006T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004006_01

Start Time:	2004-006T00:00	Stop Time:	2004-007T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004007_01

Start Time:	2004-007T00:00	Stop Time:	2004-008T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004008_01

Start Time:	2004-008T00:00	Stop Time:	2004-009T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004009_01

Start Time:	2004-009T00:00	Stop Time:	2004-010T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004010_01

Start Time:	2004-010T00:00	Stop Time:	2004-011T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004011_01

Start Time:	2004-011T00:00	Stop Time:	2004-012T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004012_01

Start Time:	2004-012T00:00	Stop Time:	2004-013T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004013_01

Start Time:	2004-013T00:00	Stop Time:	2004-014T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004014_01

Start Time:	2004-014T00:00	Stop Time:	2004-015T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004015_01

Start Time:	2004-015T00:00	Stop Time:	2004-016T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004016_01

Start Time:	2004-016T00:00	Stop Time:	2004-017T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004017_01

Start Time:	2004-017T00:00	Stop Time:	2004-018T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004018_01

Start Time:	2004-018T00:00	Stop Time:	2004-019T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004019_01

Start Time:	2004-019T00:00	Stop Time:	2004-020T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004020_01

Start Time:	2004-020T00:00	Stop Time:	2004-021T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004021_01

Start Time:	2004-021T00:00	Stop Time:	2004-022T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004022_01

Start Time:	2004-022T00:00	Stop Time:	2004-023T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004023_01

Start Time:	2004-023T00:00	Stop Time:	2004-024T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004024_01

Start Time:	2004-024T00:00	Stop Time:	2004-025T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004025_01

Start Time:	2004-025T00:00	Stop Time:	2004-026T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004026_01

Start Time:	2004-026T00:00	Stop Time:	2004-027T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004027_01

Start Time:	2004-027T00:00	Stop Time:	2004-028T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004028_01

Start Time:	2004-028T00:00	Stop Time:	2004-029T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004029_01

Start Time:	2004-029T00:00	Stop Time:	2004-030T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004030_01

Start Time:	2004-030T00:00	Stop Time:	2004-031T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004031_01

Start Time:	2004-031T00:00	Stop Time:	2004-032T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004032_01

Start Time:	2004-032T00:00	Stop Time:	2004-033T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004033_01

Start Time:	2004-033T00:00	Stop Time:	2004-034T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004034_01

Start Time:	2004-034T00:00	Stop Time:	2004-035T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004035_01

Start Time:	2004-035T00:00	Stop Time:	2004-036T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004036_01

Start Time:	2004-036T00:00	Stop Time:	2004-037T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004037_01

Start Time:	2004-037T00:00	Stop Time:	2004-038T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004038_01

Start Time:	2004-038T00:00	Stop Time:	2004-039T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004039_01

Start Time:	2004-039T00:00	Stop Time:	2004-040T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004040_01

Start Time:	2004-040T00:00	Stop Time:	2004-041T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004041_01

Start Time:	2004-041T00:00	Stop Time:	2004-042T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004042_01

Start Time:	2004-042T00:00	Stop Time:	2004-043T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004043_01

Start Time:	2004-043T00:00	Stop Time:	2004-044T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004044_01

Start Time:	2004-044T00:00	Stop Time:	2004-045T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004045_01

Start Time:	2004-045T00:00	Stop Time:	2004-046T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004046_01

Start Time:	2004-046T00:00	Stop Time:	2004-047T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004047_01

Start Time:	2004-047T00:00	Stop Time:	2004-048T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004048_01

Start Time:	2004-048T00:00	Stop Time:	2004-049T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004049_01

Start Time:	2004-049T00:00	Stop Time:	2004-050T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004050_01

Start Time:	2004-050T00:00	Stop Time:	2004-051T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004051_01

Start Time:	2004-051T00:00	Stop Time:	2004-052T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004053_01

Start Time:	2004-053T00:00	Stop Time:	2004-054T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004054_01

Start Time:	2004-054T00:00	Stop Time:	2004-055T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004055_01

Start Time:	2004-055T00:00	Stop Time:	2004-056T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004056_01

Start Time:	2004-056T00:00	Stop Time:	2004-057T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004057_01

Start Time:	2004-057T00:00	Stop Time:	2004-058T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004058_01

Start Time:	2004-058T00:00	Stop Time:	2004-059T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004059_01

Start Time:	2004-059T00:00	Stop Time:	2004-060T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004060_01

Start Time:	2004-060T00:00	Stop Time:	2004-061T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004065_01

Start Time:	2004-065T00:00	Stop Time:	2004-066T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004066_01

Start Time:	2004-066T00:00	Stop Time:	2004-067T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004067_01

Start Time:	2004-067T00:00	Stop Time:	2004-068T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004068_01

Start Time:	2004-068T00:00	Stop Time:	2004-069T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004069_01

Start Time:	2004-069T00:00	Stop Time:	2004-070T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004070_01

Start Time:	2004-070T00:00	Stop Time:	2004-071T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004071_01

Start Time:	2004-071T00:00	Stop Time:	2004-072T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004072_01

Start Time:	2004-072T00:00	Stop Time:	2004-073T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004073_01

Start Time:	2004-073T00:00	Stop Time:	2004-074T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004074_01

Start Time:	2004-074T00:00	Stop Time:	2004-075T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004075_01

Start Time:	2004-075T00:00	Stop Time:	2004-076T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004076_01

Start Time:	2004-076T00:00	Stop Time:	2004-077T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004077_01

Start Time:	2004-077T00:00	Stop Time:	2004-078T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004078_01

Start Time:	2004-078T00:00	Stop Time:	2004-079T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004079_01

Start Time:	2004-079T00:00	Stop Time:	2004-080T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004080_01

Start Time:	2004-080T00:00	Stop Time:	2004-081T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004081_01

Start Time:	2004-081T00:00	Stop Time:	2004-082T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004082_01

Start Time:	2004-082T00:00	Stop Time:	2004-083T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004083_01

Start Time:	2004-083T00:00	Stop Time:	2004-084T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004084_01

Start Time:	2004-084T00:00	Stop Time:	2004-085T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004085_01

Start Time:	2004-085T00:00	Stop Time:	2004-086T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004086_01

Start Time:	2004-086T00:00	Stop Time:	2004-087T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004087_01

Start Time:	2004-087T00:00	Stop Time:	2004-088T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004088_01

Start Time:	2004-088T00:00	Stop Time:	2004-089T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004089_01

Start Time:	2004-089T00:00	Stop Time:	2004-090T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004090_01

Start Time:	2004-090T00:00	Stop Time:	2004-091T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004091_01

Start Time:	2004-091T00:00	Stop Time:	2004-092T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004092_01

Start Time:	2004-092T00:00	Stop Time:	2004-093T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004093_01

Start Time:	2004-093T00:00	Stop Time:	2004-094T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004094_01

Start Time:	2004-094T00:00	Stop Time:	2004-095T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004095_01

Start Time:	2004-095T00:00	Stop Time:	2004-096T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004096_01

Start Time:	2004-096T00:00	Stop Time:	2004-097T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004097_01

Start Time:	2004-097T00:00	Stop Time:	2004-098T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004098_01

Start Time:	2004-098T00:00	Stop Time:	2004-099T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004099_01

Start Time:	2004-099T00:00	Stop Time:	2004-100T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004100_01

Start Time:	2004-100T00:00	Stop Time:	2004-101T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004101_01

Start Time:	2004-101T00:00	Stop Time:	2004-102T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004102_01

Start Time:	2004-102T00:00	Stop Time:	2004-103T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004103_01

Start Time:	2004-103T00:00	Stop Time:	2004-104T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004104_01

Start Time:	2004-104T00:00	Stop Time:	2004-105T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004105_01

Start Time:	2004-105T00:00	Stop Time:	2004-106T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004106_01

Start Time:	2004-106T00:00	Stop Time:	2004-107T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004107_01

Start Time:	2004-107T00:00	Stop Time:	2004-108T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004108_01

Start Time:	2004-108T00:00	Stop Time:	2004-109T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004109_01

Start Time:	2004-109T00:00	Stop Time:	2004-110T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004110_01

Start Time:	2004-110T00:00	Stop Time:	2004-111T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004111_01

Start Time:	2004-111T00:00	Stop Time:	2004-112T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004112_01

Start Time:	2004-112T00:00	Stop Time:	2004-113T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004113_01

Start Time:	2004-113T00:00	Stop Time:	2004-114T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004114_01

Start Time:	2004-114T00:00	Stop Time:	2004-115T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004115_01

Start Time:	2004-115T00:00	Stop Time:	2004-116T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004116_01

Start Time:	2004-116T00:00	Stop Time:	2004-117T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004117_01

Start Time:	2004-117T00:00	Stop Time:	2004-118T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004118_01

Start Time:	2004-118T00:00	Stop Time:	2004-119T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004119_01

Start Time:	2004-119T00:00	Stop Time:	2004-120T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004120_01

Start Time:	2004-120T00:00	Stop Time:	2004-121T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004121_01

Start Time:	2004-121T00:00	Stop Time:	2004-122T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004122_01

Start Time:	2004-122T00:00	Stop Time:	2004-123T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004123_01

Start Time:	2004-123T00:00	Stop Time:	2004-124T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004124_01

Start Time:	2004-124T00:00	Stop Time:	2004-125T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004125_01

Start Time:	2004-125T00:00	Stop Time:	2004-126T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004126_01

Start Time:	2004-126T00:00	Stop Time:	2004-127T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004127_01

Start Time:	2004-127T00:00	Stop Time:	2004-128T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004128_01

Start Time:	2004-128T00:00	Stop Time:	2004-129T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004129_01

Start Time:	2004-129T00:00	Stop Time:	2004-130T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004130_01

Start Time:	2004-130T00:00	Stop Time:	2004-131T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004131_01

Start Time:	2004-131T00:00	Stop Time:	2004-132T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004132_01

Start Time:	2004-132T00:00	Stop Time:	2004-133T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004133_01

Start Time:	2004-133T00:00	Stop Time:	2004-134T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004134_01

Start Time:	2004-134T00:00	Stop Time:	2004-135T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004135_01

Start Time:	2004-135T00:00	Stop Time:	2004-136T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004136_01

Start Time:	2004-136T00:00	Stop Time:	2004-137T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004137_01

Start Time:	2004-137T00:00	Stop Time:	2004-138T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004138_01

Start Time:	2004-138T00:00	Stop Time:	2004-139T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004139_01

Start Time:	2004-139T00:00	Stop Time:	2004-140T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004140_01

Start Time:	2004-140T00:00	Stop Time:	2004-141T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004141_01

Start Time:	2004-141T00:00	Stop Time:	2004-142T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004142_01

Start Time:	2004-142T00:00	Stop Time:	2004-143T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004143_01

Start Time:	2004-143T00:00	Stop Time:	2004-144T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004144_01

Start Time:	2004-144T00:00	Stop Time:	2004-145T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004145_01

Start Time:	2004-145T00:00	Stop Time:	2004-146T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004146_01

Start Time:	2004-146T00:00	Stop Time:	2004-147T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004147_01

Start Time:	2004-147T00:00	Stop Time:	2004-148T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004148_01

Start Time:	2004-148T00:00	Stop Time:	2004-149T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004149_01

Start Time:	2004-149T00:00	Stop Time:	2004-150T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004150_01

Start Time:	2004-150T00:00	Stop Time:	2004-151T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004151_01

Start Time:	2004-151T00:00	Stop Time:	2004-152T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004152_01

Start Time:	2004-152T00:00	Stop Time:	2004-153T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004153_01

Start Time:	2004-153T00:00	Stop Time:	2004-154T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004154_01

Start Time:	2004-154T00:00	Stop Time:	2004-155T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004155_01

Start Time:	2004-155T00:00	Stop Time:	2004-156T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004156_01

Start Time:	2004-156T00:00	Stop Time:	2004-157T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004157_01

Start Time:	2004-157T00:00	Stop Time:	2004-158T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004158_01

Start Time:	2004-158T00:00	Stop Time:	2004-159T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004159_01

Start Time:	2004-159T00:00	Stop Time:	2004-160T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004160_01

Start Time:	2004-160T00:00	Stop Time:	2004-161T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004161_01

Start Time:	2004-161T00:00	Stop Time:	2004-162T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004162_01

Start Time:	2004-162T00:00	Stop Time:	2004-163T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004163_01

Start Time:	2004-163T00:00	Stop Time:	2004-164T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004164_01

Start Time:	2004-164T00:00	Stop Time:	2004-165T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004165_01

Start Time:	2004-165T00:00	Stop Time:	2004-166T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004166_01

Start Time:	2004-166T00:00	Stop Time:	2004-167T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004167_01

Start Time:	2004-167T00:00	Stop Time:	2004-168T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004168_01

Start Time:	2004-168T00:00	Stop Time:	2004-169T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004169_01

Start Time:	2004-169T00:00	Stop Time:	2004-170T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004170_01

Start Time:	2004-170T00:00	Stop Time:	2004-171T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004171_01

Start Time:	2004-171T00:00	Stop Time:	2004-172T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004172_01

Start Time:	2004-172T00:00	Stop Time:	2004-173T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004173_01

Start Time:	2004-173T00:00	Stop Time:	2004-174T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004174_01

Start Time:	2004-174T00:00	Stop Time:	2004-175T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004175_01

Start Time:	2004-175T00:00	Stop Time:	2004-176T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004176_01

Start Time:	2004-176T00:00	Stop Time:	2004-177T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004177_01

Start Time:	2004-177T00:00	Stop Time:	2004-178T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004178_01

Start Time:	2004-178T00:00	Stop Time:	2004-179T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004179_01

Start Time:	2004-179T00:00	Stop Time:	2004-180T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004180_01

Start Time:	2004-180T00:00	Stop Time:	2004-181T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004181_01

Start Time:	2004-181T00:00	Stop Time:	2004-182T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004182_01

Start Time:	2004-182T00:00	Stop Time:	2004-183T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004183_01

Start Time:	2004-183T00:00	Stop Time:	2004-184T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004184_01

Start Time:	2004-184T00:00	Stop Time:	2004-185T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004185_01

Start Time:	2004-185T00:00	Stop Time:	2004-186T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004186_01

Start Time:	2004-186T00:00	Stop Time:	2004-187T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004194_01

Start Time:	2004-194T00:00	Stop Time:	2004-195T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004195_01

Start Time:	2004-195T00:00	Stop Time:	2004-196T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004196_01

Start Time:	2004-196T00:00	Stop Time:	2004-197T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004197_01

Start Time:	2004-197T00:00	Stop Time:	2004-198T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004198_01

Start Time:	2004-198T00:00	Stop Time:	2004-199T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004199_01

Start Time:	2004-199T00:00	Stop Time:	2004-200T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004200_01

Start Time:	2004-200T00:00	Stop Time:	2004-201T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004201_01

Start Time:	2004-201T00:00	Stop Time:	2004-202T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004202_01

Start Time:	2004-202T00:00	Stop Time:	2004-203T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004203_01

Start Time:	2004-203T00:00	Stop Time:	2004-204T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004204_01

Start Time:	2004-204T00:00	Stop Time:	2004-205T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004205_01

Start Time:	2004-205T00:00	Stop Time:	2004-206T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004206_01

Start Time:	2004-206T00:00	Stop Time:	2004-207T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004207_01

Start Time:	2004-207T00:00	Stop Time:	2004-208T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004208_01

Start Time:	2004-208T00:00	Stop Time:	2004-209T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004209_01

Start Time:	2004-209T00:00	Stop Time:	2004-210T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004210_01

Start Time:	2004-210T00:00	Stop Time:	2004-211T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004211_01

Start Time:	2004-211T00:00	Stop Time:	2004-212T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004212_01

Start Time:	2004-212T00:00	Stop Time:	2004-213T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004213_01

Start Time:	2004-213T00:00	Stop Time:	2004-214T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004214_01

Start Time:	2004-214T00:00	Stop Time:	2004-215T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004215_01

Start Time:	2004-215T00:00	Stop Time:	2004-216T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004216_01

Start Time:	2004-216T00:00	Stop Time:	2004-217T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004217_01

Start Time:	2004-217T00:00	Stop Time:	2004-218T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004218_01

Start Time:	2004-218T00:00	Stop Time:	2004-219T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004219_01

Start Time:	2004-219T00:00	Stop Time:	2004-220T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004220_01

Start Time:	2004-220T00:00	Stop Time:	2004-221T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004221_01

Start Time:	2004-221T00:00	Stop Time:	2004-222T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004222_01

Start Time:	2004-222T00:00	Stop Time:	2004-223T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004223_01

Start Time:	2004-223T00:00	Stop Time:	2004-224T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004224_01

Start Time:	2004-224T00:00	Stop Time:	2004-225T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004225_01

Start Time:	2004-225T00:00	Stop Time:	2004-226T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004226_01

Start Time:	2004-226T00:00	Stop Time:	2004-227T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004227_01

Start Time:	2004-227T00:00	Stop Time:	2004-228T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004228_01

Start Time:	2004-228T00:00	Stop Time:	2004-229T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004229_01

Start Time:	2004-229T00:00	Stop Time:	2004-230T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004230_01

Start Time:	2004-230T00:00	Stop Time:	2004-231T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004231_01

Start Time:	2004-231T00:00	Stop Time:	2004-232T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004232_01

Start Time:	2004-232T00:00	Stop Time:	2004-233T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004233_01

Start Time:	2004-233T00:00	Stop Time:	2004-234T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004234_01

Start Time:	2004-234T00:00	Stop Time:	2004-235T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004235_01

Start Time:	2004-235T00:00	Stop Time:	2004-236T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004236_01

Start Time:	2004-236T00:00	Stop Time:	2004-237T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004237_01

Start Time:	2004-237T00:00	Stop Time:	2004-238T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004238_01

Start Time:	2004-238T00:00	Stop Time:	2004-239T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004239_01

Start Time:	2004-239T00:00	Stop Time:	2004-240T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004240_01

Start Time:	2004-240T00:00	Stop Time:	2004-241T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004241_01

Start Time:	2004-241T00:00	Stop Time:	2004-242T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004242_01

Start Time:	2004-242T00:00	Stop Time:	2004-243T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004243_01

Start Time:	2004-243T00:00	Stop Time:	2004-244T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004244_01

Start Time:	2004-244T00:00	Stop Time:	2004-245T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004245_01

Start Time:	2004-245T00:00	Stop Time:	2004-246T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004246_01

Start Time:	2004-246T00:00	Stop Time:	2004-247T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004247_01

Start Time:	2004-247T00:00	Stop Time:	2004-248T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004248_01

Start Time:	2004-248T00:00	Stop Time:	2004-249T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004249_01

Start Time:	2004-249T00:00	Stop Time:	2004-250T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004250_01

Start Time:	2004-250T00:00	Stop Time:	2004-251T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004251_01

Start Time:	2004-251T00:00	Stop Time:	2004-252T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004252_01

Start Time:	2004-252T00:00	Stop Time:	2004-253T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004253_01

Start Time:	2004-253T00:00	Stop Time:	2004-254T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004254_01

Start Time:	2004-254T00:00	Stop Time:	2004-255T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004255_01

Start Time:	2004-255T00:00	Stop Time:	2004-256T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004256_01

Start Time:	2004-256T00:00	Stop Time:	2004-257T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004257_01

Start Time:	2004-257T00:00	Stop Time:	2004-258T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004258_01

Start Time:	2004-258T00:00	Stop Time:	2004-259T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004259_01

Start Time:	2004-259T00:00	Stop Time:	2004-260T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004260_01

Start Time:	2004-260T00:00	Stop Time:	2004-261T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004261_01

Start Time:	2004-261T00:00	Stop Time:	2004-262T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004262_01

Start Time:	2004-262T00:00	Stop Time:	2004-263T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004263_01

Start Time:	2004-263T00:00	Stop Time:	2004-264T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004264_01

Start Time:	2004-264T00:00	Stop Time:	2004-265T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004265_01

Start Time:	2004-265T00:00	Stop Time:	2004-266T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004266_01

Start Time:	2004-266T00:00	Stop Time:	2004-267T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004267_01

Start Time:	2004-267T00:00	Stop Time:	2004-268T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004268_01

Start Time:	2004-268T00:00	Stop Time:	2004-269T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004269_01

Start Time:	2004-269T00:00	Stop Time:	2004-270T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004270_01

Start Time:	2004-270T00:00	Stop Time:	2004-271T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004271_01

Start Time:	2004-271T00:00	Stop Time:	2004-272T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004272_01

Start Time:	2004-272T00:00	Stop Time:	2004-273T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004273_01

Start Time:	2004-273T00:00	Stop Time:	2004-274T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004274_01

Start Time:	2004-274T00:00	Stop Time:	2004-275T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004275_01

Start Time:	2004-275T00:00	Stop Time:	2004-276T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004276_01

Start Time:	2004-276T00:00	Stop Time:	2004-277T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004277_01

Start Time:	2004-277T00:00	Stop Time:	2004-278T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004278_01

Start Time:	2004-278T00:00	Stop Time:	2004-279T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004279_01

Start Time:	2004-279T00:00	Stop Time:	2004-280T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004280_01

Start Time:	2004-280T00:00	Stop Time:	2004-281T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004281_01

Start Time:	2004-281T00:00	Stop Time:	2004-282T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004282_01

Start Time:	2004-282T00:00	Stop Time:	2004-283T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004283_01

Start Time:	2004-283T00:00	Stop Time:	2004-284T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004284_01

Start Time:	2004-284T00:00	Stop Time:	2004-285T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004285_01

Start Time:	2004-285T00:00	Stop Time:	2004-286T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004286_01

Start Time:	2004-286T00:00	Stop Time:	2004-287T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004287_01

Start Time:	2004-287T00:00	Stop Time:	2004-288T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004288_01

Start Time:	2004-288T00:00	Stop Time:	2004-289T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004289_01

Start Time:	2004-289T00:00	Stop Time:	2004-290T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004290_01

Start Time:	2004-290T00:00	Stop Time:	2004-291T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004291_01

Start Time:	2004-291T00:00	Stop Time:	2004-292T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004292_01

Start Time:	2004-292T00:00	Stop Time:	2004-293T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004293_01

Start Time:	2004-293T00:00	Stop Time:	2004-294T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004294_01

Start Time:	2004-294T00:00	Stop Time:	2004-295T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004295_01

Start Time:	2004-295T00:00	Stop Time:	2004-296T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004296_01

Start Time:	2004-296T00:00	Stop Time:	2004-297T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004297_01

Start Time:	2004-297T00:00	Stop Time:	2004-298T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004298_01

Start Time:	2004-298T00:00	Stop Time:	2004-299T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004299_01

Start Time:	2004-299T00:00	Stop Time:	2004-300T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004300_01

Start Time:	2004-300T00:00	Stop Time:	2004-301T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004301_01

Start Time:	2004-301T00:00	Stop Time:	2004-302T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004302_01

Start Time:	2004-302T00:00	Stop Time:	2004-303T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004303_01

Start Time:	2004-303T00:00	Stop Time:	2004-304T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004304_01

Start Time:	2004-304T00:00	Stop Time:	2004-305T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004305_01

Start Time:	2004-305T00:00	Stop Time:	2004-306T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004306_01

Start Time:	2004-306T00:00	Stop Time:	2004-307T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004307_01

Start Time:	2004-307T00:00	Stop Time:	2004-308T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004308_01

Start Time:	2004-308T00:00	Stop Time:	2004-309T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004309_01

Start Time:	2004-309T00:00	Stop Time:	2004-310T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004310_01

Start Time:	2004-310T00:00	Stop Time:	2004-311T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004311_01

Start Time:	2004-311T00:00	Stop Time:	2004-312T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004312_01

Start Time:	2004-312T00:00	Stop Time:	2004-313T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004313_01

Start Time:	2004-313T00:00	Stop Time:	2004-314T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004314_01

Start Time:	2004-314T00:00	Stop Time:	2004-315T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004315_01

Start Time:	2004-315T00:00	Stop Time:	2004-316T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004316_01

Start Time:	2004-316T00:00	Stop Time:	2004-317T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004317_01

Start Time:	2004-317T00:00	Stop Time:	2004-318T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004318_01

Start Time:	2004-318T00:00	Stop Time:	2004-319T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004319_01

Start Time:	2004-319T00:00	Stop Time:	2004-320T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004320_01

Start Time:	2004-320T00:00	Stop Time:	2004-321T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004321_01

Start Time:	2004-321T00:00	Stop Time:	2004-322T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004322_01

Start Time:	2004-322T00:00	Stop Time:	2004-323T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004323_01

Start Time:	2004-323T00:00	Stop Time:	2004-324T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004324_01

Start Time:	2004-324T00:00	Stop Time:	2004-325T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004325_01

Start Time:	2004-325T00:00	Stop Time:	2004-326T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004326_01

Start Time:	2004-326T00:00	Stop Time:	2004-327T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004327_01

Start Time:	2004-327T00:00	Stop Time:	2004-328T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004328_01

Start Time:	2004-328T00:00	Stop Time:	2004-329T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004329_01

Start Time:	2004-329T00:00	Stop Time:	2004-330T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004330_01

Start Time:	2004-330T00:00	Stop Time:	2004-331T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004331_01

Start Time:	2004-331T00:00	Stop Time:	2004-332T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004332_01

Start Time:	2004-332T00:00	Stop Time:	2004-333T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004333_01

Start Time:	2004-333T00:00	Stop Time:	2004-334T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004334_01

Start Time:	2004-334T00:00	Stop Time:	2004-335T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004335_01

Start Time:	2004-335T00:00	Stop Time:	2004-336T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004336_01

Start Time:	2004-336T00:00	Stop Time:	2004-337T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004337_01

Start Time:	2004-337T00:00	Stop Time:	2004-338T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004338_01

Start Time:	2004-338T00:00	Stop Time:	2004-339T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004339_01

Start Time:	2004-339T00:00	Stop Time:	2004-340T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004340_01

Start Time:	2004-340T00:00	Stop Time:	2004-341T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004341_01

Start Time:	2004-341T00:00	Stop Time:	2004-342T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004342_01

Start Time:	2004-342T00:00	Stop Time:	2004-343T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004343_01

Start Time:	2004-343T00:00	Stop Time:	2004-344T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004344_01

Start Time:	2004-344T00:00	Stop Time:	2004-345T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004345_01

Start Time:	2004-345T00:00	Stop Time:	2004-346T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004346_01

Start Time:	2004-346T00:00	Stop Time:	2004-347T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004347_01

Start Time:	2004-347T00:00	Stop Time:	2004-348T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004348_01

Start Time:	2004-348T00:00	Stop Time:	2004-349T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004349_01

Start Time:	2004-349T00:00	Stop Time:	2004-350T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004350_01

Start Time:	2004-350T00:00	Stop Time:	2004-351T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004351_01

Start Time:	2004-351T00:00	Stop Time:	2004-352T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004352_01

Start Time:	2004-352T00:00	Stop Time:	2004-353T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004353_01

Start Time:	2004-353T00:00	Stop Time:	2004-354T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004354_01

Start Time:	2004-354T00:00	Stop Time:	2004-355T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004355_01

Start Time:	2004-355T00:00	Stop Time:	2004-356T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004356_01

Start Time:	2004-356T00:00	Stop Time:	2004-357T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004357_01

Start Time:	2004-357T00:00	Stop Time:	2004-358T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004358_01

Start Time:	2004-358T00:00	Stop Time:	2004-359T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004359_01

Start Time:	2004-359T00:00	Stop Time:	2004-360T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004360_01

Start Time:	2004-360T00:00	Stop Time:	2004-361T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004361_01

Start Time:	2004-361T00:00	Stop Time:	2004-362T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004362_01

Start Time:	2004-362T00:00	Stop Time:	2004-363T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004363_01

Start Time:	2004-363T00:00	Stop Time:	2004-364T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004364_01

Start Time:	2004-364T00:00	Stop Time:	2004-365T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004365_01

Start Time:	2004-365T00:00	Stop Time:	2004-366T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LPHAAVG0_1MIN_2004366_01

Start Time:	2004-366T00:00	Stop Time:	2005-001T00:00
The data columns contain 1 minute averages of LEMMS PHA data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

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