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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/ LACCAVG0_1MIN/ 2005 /

LACCAVG0_1MIN_2005001_01

Start Time:	2005-001T00:00	Stop Time:	2005-002T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005002_01

Start Time:	2005-002T00:00	Stop Time:	2005-003T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005003_01

Start Time:	2005-003T00:00	Stop Time:	2005-004T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005004_01

Start Time:	2005-004T00:00	Stop Time:	2005-005T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005005_01

Start Time:	2005-005T00:00	Stop Time:	2005-006T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005006_01

Start Time:	2005-006T00:00	Stop Time:	2005-007T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005015_01

Start Time:	2005-015T00:00	Stop Time:	2005-016T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005016_01

Start Time:	2005-016T00:00	Stop Time:	2005-017T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005017_01

Start Time:	2005-017T00:00	Stop Time:	2005-018T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005018_01

Start Time:	2005-018T00:00	Stop Time:	2005-019T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005019_01

Start Time:	2005-019T00:00	Stop Time:	2005-020T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005020_01

Start Time:	2005-020T00:00	Stop Time:	2005-021T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005021_01

Start Time:	2005-021T00:00	Stop Time:	2005-022T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005022_01

Start Time:	2005-022T00:00	Stop Time:	2005-023T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005023_01

Start Time:	2005-023T00:00	Stop Time:	2005-024T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005024_01

Start Time:	2005-024T00:00	Stop Time:	2005-025T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005025_01

Start Time:	2005-025T00:00	Stop Time:	2005-026T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005026_01

Start Time:	2005-026T00:00	Stop Time:	2005-027T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005027_01

Start Time:	2005-027T00:00	Stop Time:	2005-028T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005028_01

Start Time:	2005-028T00:00	Stop Time:	2005-029T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005029_01

Start Time:	2005-029T00:00	Stop Time:	2005-030T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005030_01

Start Time:	2005-030T00:00	Stop Time:	2005-031T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005031_01

Start Time:	2005-031T00:00	Stop Time:	2005-032T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005032_01

Start Time:	2005-032T00:00	Stop Time:	2005-033T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005033_01

Start Time:	2005-033T00:00	Stop Time:	2005-034T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005034_01

Start Time:	2005-034T00:00	Stop Time:	2005-035T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005035_01

Start Time:	2005-035T00:00	Stop Time:	2005-036T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005036_01

Start Time:	2005-036T00:00	Stop Time:	2005-037T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005037_01

Start Time:	2005-037T00:00	Stop Time:	2005-038T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005038_01

Start Time:	2005-038T00:00	Stop Time:	2005-039T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005039_01

Start Time:	2005-039T00:00	Stop Time:	2005-040T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005040_01

Start Time:	2005-040T00:00	Stop Time:	2005-041T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005041_01

Start Time:	2005-041T00:00	Stop Time:	2005-042T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005042_01

Start Time:	2005-042T00:00	Stop Time:	2005-043T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005043_01

Start Time:	2005-043T00:00	Stop Time:	2005-044T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005044_01

Start Time:	2005-044T00:00	Stop Time:	2005-045T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005045_01

Start Time:	2005-045T00:00	Stop Time:	2005-046T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005046_01

Start Time:	2005-046T00:00	Stop Time:	2005-047T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005047_01

Start Time:	2005-047T00:00	Stop Time:	2005-048T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005048_01

Start Time:	2005-048T00:00	Stop Time:	2005-049T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005049_01

Start Time:	2005-049T00:00	Stop Time:	2005-050T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005050_01

Start Time:	2005-050T00:00	Stop Time:	2005-051T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005051_01

Start Time:	2005-051T00:00	Stop Time:	2005-052T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005052_01

Start Time:	2005-052T00:00	Stop Time:	2005-053T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005053_01

Start Time:	2005-053T00:00	Stop Time:	2005-054T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005054_01

Start Time:	2005-054T00:00	Stop Time:	2005-055T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005055_01

Start Time:	2005-055T00:00	Stop Time:	2005-056T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005056_01

Start Time:	2005-056T00:00	Stop Time:	2005-057T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005057_01

Start Time:	2005-057T00:00	Stop Time:	2005-058T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005058_01

Start Time:	2005-058T00:00	Stop Time:	2005-059T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005059_01

Start Time:	2005-059T00:00	Stop Time:	2005-060T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005060_01

Start Time:	2005-060T00:00	Stop Time:	2005-061T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005061_01

Start Time:	2005-061T00:00	Stop Time:	2005-062T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005062_01

Start Time:	2005-062T00:00	Stop Time:	2005-063T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005063_01

Start Time:	2005-063T00:00	Stop Time:	2005-064T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005064_01

Start Time:	2005-064T00:00	Stop Time:	2005-065T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005065_01

Start Time:	2005-065T00:00	Stop Time:	2005-066T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005066_01

Start Time:	2005-066T00:00	Stop Time:	2005-067T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005067_01

Start Time:	2005-067T00:00	Stop Time:	2005-068T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005068_01

Start Time:	2005-068T00:00	Stop Time:	2005-069T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005069_01

Start Time:	2005-069T00:00	Stop Time:	2005-070T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005070_01

Start Time:	2005-070T00:00	Stop Time:	2005-071T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005071_01

Start Time:	2005-071T00:00	Stop Time:	2005-072T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005072_01

Start Time:	2005-072T00:00	Stop Time:	2005-073T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005073_01

Start Time:	2005-073T00:00	Stop Time:	2005-074T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005074_01

Start Time:	2005-074T00:00	Stop Time:	2005-075T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005075_01

Start Time:	2005-075T00:00	Stop Time:	2005-076T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005076_01

Start Time:	2005-076T00:00	Stop Time:	2005-077T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005077_01

Start Time:	2005-077T00:00	Stop Time:	2005-078T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005078_01

Start Time:	2005-078T00:00	Stop Time:	2005-079T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005079_01

Start Time:	2005-079T00:00	Stop Time:	2005-080T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005080_01

Start Time:	2005-080T00:00	Stop Time:	2005-081T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005081_01

Start Time:	2005-081T00:00	Stop Time:	2005-082T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005082_01

Start Time:	2005-082T00:00	Stop Time:	2005-083T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005083_01

Start Time:	2005-083T00:00	Stop Time:	2005-084T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005084_01

Start Time:	2005-084T00:00	Stop Time:	2005-085T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005085_01

Start Time:	2005-085T00:00	Stop Time:	2005-086T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005086_01

Start Time:	2005-086T00:00	Stop Time:	2005-087T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005087_01

Start Time:	2005-087T00:00	Stop Time:	2005-088T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005088_01

Start Time:	2005-088T00:00	Stop Time:	2005-089T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005089_01

Start Time:	2005-089T00:00	Stop Time:	2005-090T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005090_01

Start Time:	2005-090T00:00	Stop Time:	2005-091T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005091_01

Start Time:	2005-091T00:00	Stop Time:	2005-092T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005092_01

Start Time:	2005-092T00:00	Stop Time:	2005-093T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005093_01

Start Time:	2005-093T00:00	Stop Time:	2005-094T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005094_01

Start Time:	2005-094T00:00	Stop Time:	2005-095T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005095_01

Start Time:	2005-095T00:00	Stop Time:	2005-096T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005096_01

Start Time:	2005-096T00:00	Stop Time:	2005-097T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005097_01

Start Time:	2005-097T00:00	Stop Time:	2005-098T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005098_01

Start Time:	2005-098T00:00	Stop Time:	2005-099T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005099_01

Start Time:	2005-099T00:00	Stop Time:	2005-100T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005100_01

Start Time:	2005-100T00:00	Stop Time:	2005-101T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005101_01

Start Time:	2005-101T00:00	Stop Time:	2005-102T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005102_01

Start Time:	2005-102T00:00	Stop Time:	2005-103T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005103_01

Start Time:	2005-103T00:00	Stop Time:	2005-104T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005104_01

Start Time:	2005-104T00:00	Stop Time:	2005-105T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005105_01

Start Time:	2005-105T00:00	Stop Time:	2005-106T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005106_01

Start Time:	2005-106T00:00	Stop Time:	2005-107T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005107_01

Start Time:	2005-107T00:00	Stop Time:	2005-108T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005108_01

Start Time:	2005-108T00:00	Stop Time:	2005-109T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005109_01

Start Time:	2005-109T00:00	Stop Time:	2005-110T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005110_01

Start Time:	2005-110T00:00	Stop Time:	2005-111T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005111_01

Start Time:	2005-111T00:00	Stop Time:	2005-112T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005112_01

Start Time:	2005-112T00:00	Stop Time:	2005-113T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005113_01

Start Time:	2005-113T00:00	Stop Time:	2005-114T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005114_01

Start Time:	2005-114T00:00	Stop Time:	2005-115T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005115_01

Start Time:	2005-115T00:00	Stop Time:	2005-116T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005116_01

Start Time:	2005-116T00:00	Stop Time:	2005-117T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005117_01

Start Time:	2005-117T00:00	Stop Time:	2005-118T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005118_01

Start Time:	2005-118T00:00	Stop Time:	2005-119T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005119_01

Start Time:	2005-119T00:00	Stop Time:	2005-120T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005120_01

Start Time:	2005-120T00:00	Stop Time:	2005-121T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005121_01

Start Time:	2005-121T00:00	Stop Time:	2005-122T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005122_01

Start Time:	2005-122T00:00	Stop Time:	2005-123T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005123_01

Start Time:	2005-123T00:00	Stop Time:	2005-124T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005124_01

Start Time:	2005-124T00:00	Stop Time:	2005-125T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005125_01

Start Time:	2005-125T00:00	Stop Time:	2005-126T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005126_01

Start Time:	2005-126T00:00	Stop Time:	2005-127T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005127_01

Start Time:	2005-127T00:00	Stop Time:	2005-128T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005128_01

Start Time:	2005-128T00:00	Stop Time:	2005-129T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005129_01

Start Time:	2005-129T00:00	Stop Time:	2005-130T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005130_01

Start Time:	2005-130T00:00	Stop Time:	2005-131T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005131_01

Start Time:	2005-131T00:00	Stop Time:	2005-132T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005132_01

Start Time:	2005-132T00:00	Stop Time:	2005-133T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005133_01

Start Time:	2005-133T00:00	Stop Time:	2005-134T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005134_01

Start Time:	2005-134T00:00	Stop Time:	2005-135T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005135_01

Start Time:	2005-135T00:00	Stop Time:	2005-136T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005136_01

Start Time:	2005-136T00:00	Stop Time:	2005-137T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005137_01

Start Time:	2005-137T00:00	Stop Time:	2005-138T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005138_01

Start Time:	2005-138T00:00	Stop Time:	2005-139T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005139_01

Start Time:	2005-139T00:00	Stop Time:	2005-140T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005140_01

Start Time:	2005-140T00:00	Stop Time:	2005-141T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005141_01

Start Time:	2005-141T00:00	Stop Time:	2005-142T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005142_01

Start Time:	2005-142T00:00	Stop Time:	2005-143T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005143_01

Start Time:	2005-143T00:00	Stop Time:	2005-144T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005144_01

Start Time:	2005-144T00:00	Stop Time:	2005-145T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005145_01

Start Time:	2005-145T00:00	Stop Time:	2005-146T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005146_01

Start Time:	2005-146T00:00	Stop Time:	2005-147T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005147_01

Start Time:	2005-147T00:00	Stop Time:	2005-148T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005148_01

Start Time:	2005-148T00:00	Stop Time:	2005-149T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005149_01

Start Time:	2005-149T00:00	Stop Time:	2005-150T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005150_01

Start Time:	2005-150T00:00	Stop Time:	2005-151T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005151_01

Start Time:	2005-151T00:00	Stop Time:	2005-152T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005152_01

Start Time:	2005-152T00:00	Stop Time:	2005-153T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005153_01

Start Time:	2005-153T00:00	Stop Time:	2005-154T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005154_01

Start Time:	2005-154T00:00	Stop Time:	2005-155T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005155_01

Start Time:	2005-155T00:00	Stop Time:	2005-156T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005156_01

Start Time:	2005-156T00:00	Stop Time:	2005-157T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005157_01

Start Time:	2005-157T00:00	Stop Time:	2005-158T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005158_01

Start Time:	2005-158T00:00	Stop Time:	2005-159T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005159_01

Start Time:	2005-159T00:00	Stop Time:	2005-160T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005160_01

Start Time:	2005-160T00:00	Stop Time:	2005-161T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005161_01

Start Time:	2005-161T00:00	Stop Time:	2005-162T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005162_01

Start Time:	2005-162T00:00	Stop Time:	2005-163T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005163_01

Start Time:	2005-163T00:00	Stop Time:	2005-164T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005164_01

Start Time:	2005-164T00:00	Stop Time:	2005-165T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005165_01

Start Time:	2005-165T00:00	Stop Time:	2005-166T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005166_01

Start Time:	2005-166T00:00	Stop Time:	2005-167T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005167_01

Start Time:	2005-167T00:00	Stop Time:	2005-168T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005168_01

Start Time:	2005-168T00:00	Stop Time:	2005-169T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005169_01

Start Time:	2005-169T00:00	Stop Time:	2005-170T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005170_01

Start Time:	2005-170T00:00	Stop Time:	2005-171T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005171_01

Start Time:	2005-171T00:00	Stop Time:	2005-172T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005172_01

Start Time:	2005-172T00:00	Stop Time:	2005-173T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005173_01

Start Time:	2005-173T00:00	Stop Time:	2005-174T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005174_01

Start Time:	2005-174T00:00	Stop Time:	2005-175T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005175_01

Start Time:	2005-175T00:00	Stop Time:	2005-176T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005176_01

Start Time:	2005-176T00:00	Stop Time:	2005-177T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005177_01

Start Time:	2005-177T00:00	Stop Time:	2005-178T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005178_01

Start Time:	2005-178T00:00	Stop Time:	2005-179T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005179_01

Start Time:	2005-179T00:00	Stop Time:	2005-180T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005180_01

Start Time:	2005-180T00:00	Stop Time:	2005-181T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005181_01

Start Time:	2005-181T00:00	Stop Time:	2005-182T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005182_01

Start Time:	2005-182T00:00	Stop Time:	2005-183T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005183_01

Start Time:	2005-183T00:00	Stop Time:	2005-184T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005184_01

Start Time:	2005-184T00:00	Stop Time:	2005-185T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005185_01

Start Time:	2005-185T00:00	Stop Time:	2005-186T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005186_01

Start Time:	2005-186T00:00	Stop Time:	2005-187T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005187_01

Start Time:	2005-187T00:00	Stop Time:	2005-188T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005188_01

Start Time:	2005-188T00:00	Stop Time:	2005-189T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005189_01

Start Time:	2005-189T00:00	Stop Time:	2005-190T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005190_01

Start Time:	2005-190T00:00	Stop Time:	2005-191T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005191_01

Start Time:	2005-191T00:00	Stop Time:	2005-192T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005192_01

Start Time:	2005-192T00:00	Stop Time:	2005-193T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005193_01

Start Time:	2005-193T00:00	Stop Time:	2005-194T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005194_01

Start Time:	2005-194T00:00	Stop Time:	2005-195T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005195_01

Start Time:	2005-195T00:00	Stop Time:	2005-196T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005196_01

Start Time:	2005-196T00:00	Stop Time:	2005-197T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005197_01

Start Time:	2005-197T00:00	Stop Time:	2005-198T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005198_01

Start Time:	2005-198T00:00	Stop Time:	2005-199T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005199_01

Start Time:	2005-199T00:00	Stop Time:	2005-200T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005200_01

Start Time:	2005-200T00:00	Stop Time:	2005-201T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005201_01

Start Time:	2005-201T00:00	Stop Time:	2005-202T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005202_01

Start Time:	2005-202T00:00	Stop Time:	2005-203T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005203_01

Start Time:	2005-203T00:00	Stop Time:	2005-204T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005204_01

Start Time:	2005-204T00:00	Stop Time:	2005-205T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005205_01

Start Time:	2005-205T00:00	Stop Time:	2005-206T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005206_01

Start Time:	2005-206T00:00	Stop Time:	2005-207T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005207_01

Start Time:	2005-207T00:00	Stop Time:	2005-208T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005208_01

Start Time:	2005-208T00:00	Stop Time:	2005-209T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005209_01

Start Time:	2005-209T00:00	Stop Time:	2005-210T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005210_01

Start Time:	2005-210T00:00	Stop Time:	2005-211T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005211_01

Start Time:	2005-211T00:00	Stop Time:	2005-212T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005212_01

Start Time:	2005-212T00:00	Stop Time:	2005-213T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005213_01

Start Time:	2005-213T00:00	Stop Time:	2005-214T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005214_01

Start Time:	2005-214T00:00	Stop Time:	2005-215T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005215_01

Start Time:	2005-215T00:00	Stop Time:	2005-216T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005216_01

Start Time:	2005-216T00:00	Stop Time:	2005-217T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005217_01

Start Time:	2005-217T00:00	Stop Time:	2005-218T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005218_01

Start Time:	2005-218T00:00	Stop Time:	2005-219T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005219_01

Start Time:	2005-219T00:00	Stop Time:	2005-220T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005220_01

Start Time:	2005-220T00:00	Stop Time:	2005-221T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005221_01

Start Time:	2005-221T00:00	Stop Time:	2005-222T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005222_01

Start Time:	2005-222T00:00	Stop Time:	2005-223T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005223_01

Start Time:	2005-223T00:00	Stop Time:	2005-224T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005224_01

Start Time:	2005-224T00:00	Stop Time:	2005-225T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005225_01

Start Time:	2005-225T00:00	Stop Time:	2005-226T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005226_01

Start Time:	2005-226T00:00	Stop Time:	2005-227T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005227_01

Start Time:	2005-227T00:00	Stop Time:	2005-228T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005228_01

Start Time:	2005-228T00:00	Stop Time:	2005-229T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005229_01

Start Time:	2005-229T00:00	Stop Time:	2005-230T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005230_01

Start Time:	2005-230T00:00	Stop Time:	2005-231T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005231_01

Start Time:	2005-231T00:00	Stop Time:	2005-232T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005232_01

Start Time:	2005-232T00:00	Stop Time:	2005-233T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005233_01

Start Time:	2005-233T00:00	Stop Time:	2005-234T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005234_01

Start Time:	2005-234T00:00	Stop Time:	2005-235T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005235_01

Start Time:	2005-235T00:00	Stop Time:	2005-236T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005236_01

Start Time:	2005-236T00:00	Stop Time:	2005-237T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005237_01

Start Time:	2005-237T00:00	Stop Time:	2005-238T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005238_01

Start Time:	2005-238T00:00	Stop Time:	2005-239T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005239_01

Start Time:	2005-239T00:00	Stop Time:	2005-240T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005240_01

Start Time:	2005-240T00:00	Stop Time:	2005-241T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005241_01

Start Time:	2005-241T00:00	Stop Time:	2005-242T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005242_01

Start Time:	2005-242T00:00	Stop Time:	2005-243T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005243_01

Start Time:	2005-243T00:00	Stop Time:	2005-244T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005244_01

Start Time:	2005-244T00:00	Stop Time:	2005-245T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005245_01

Start Time:	2005-245T00:00	Stop Time:	2005-246T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005246_01

Start Time:	2005-246T00:00	Stop Time:	2005-247T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005247_01

Start Time:	2005-247T00:00	Stop Time:	2005-248T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005248_01

Start Time:	2005-248T00:00	Stop Time:	2005-249T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005249_01

Start Time:	2005-249T00:00	Stop Time:	2005-250T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005250_01

Start Time:	2005-250T00:00	Stop Time:	2005-251T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005251_01

Start Time:	2005-251T00:00	Stop Time:	2005-252T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005252_01

Start Time:	2005-252T00:00	Stop Time:	2005-253T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005253_01

Start Time:	2005-253T00:00	Stop Time:	2005-254T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005254_01

Start Time:	2005-254T00:00	Stop Time:	2005-255T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005255_01

Start Time:	2005-255T00:00	Stop Time:	2005-256T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005256_01

Start Time:	2005-256T00:00	Stop Time:	2005-257T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005257_01

Start Time:	2005-257T00:00	Stop Time:	2005-258T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005258_01

Start Time:	2005-258T00:00	Stop Time:	2005-259T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005259_01

Start Time:	2005-259T00:00	Stop Time:	2005-260T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005260_01

Start Time:	2005-260T00:00	Stop Time:	2005-261T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005261_01

Start Time:	2005-261T00:00	Stop Time:	2005-262T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005262_01

Start Time:	2005-262T00:00	Stop Time:	2005-263T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005263_01

Start Time:	2005-263T00:00	Stop Time:	2005-264T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005264_01

Start Time:	2005-264T00:00	Stop Time:	2005-265T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005265_01

Start Time:	2005-265T00:00	Stop Time:	2005-266T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005266_01

Start Time:	2005-266T00:00	Stop Time:	2005-267T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005267_01

Start Time:	2005-267T00:00	Stop Time:	2005-268T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005268_01

Start Time:	2005-268T00:00	Stop Time:	2005-269T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005269_01

Start Time:	2005-269T00:00	Stop Time:	2005-270T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005270_01

Start Time:	2005-270T00:00	Stop Time:	2005-271T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005271_01

Start Time:	2005-271T00:00	Stop Time:	2005-272T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005272_01

Start Time:	2005-272T00:00	Stop Time:	2005-273T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005273_01

Start Time:	2005-273T00:00	Stop Time:	2005-274T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005274_01

Start Time:	2005-274T00:00	Stop Time:	2005-275T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005275_01

Start Time:	2005-275T00:00	Stop Time:	2005-276T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005276_01

Start Time:	2005-276T00:00	Stop Time:	2005-277T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005277_01

Start Time:	2005-277T00:00	Stop Time:	2005-278T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005278_01

Start Time:	2005-278T00:00	Stop Time:	2005-279T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005279_01

Start Time:	2005-279T00:00	Stop Time:	2005-280T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005280_01

Start Time:	2005-280T00:00	Stop Time:	2005-281T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005281_01

Start Time:	2005-281T00:00	Stop Time:	2005-282T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005282_01

Start Time:	2005-282T00:00	Stop Time:	2005-283T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005283_01

Start Time:	2005-283T00:00	Stop Time:	2005-284T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005284_01

Start Time:	2005-284T00:00	Stop Time:	2005-285T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005285_01

Start Time:	2005-285T00:00	Stop Time:	2005-286T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005286_01

Start Time:	2005-286T00:00	Stop Time:	2005-287T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005287_01

Start Time:	2005-287T00:00	Stop Time:	2005-288T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005288_01

Start Time:	2005-288T00:00	Stop Time:	2005-289T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005289_01

Start Time:	2005-289T00:00	Stop Time:	2005-290T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005290_01

Start Time:	2005-290T00:00	Stop Time:	2005-291T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005291_01

Start Time:	2005-291T00:00	Stop Time:	2005-292T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005292_01

Start Time:	2005-292T00:00	Stop Time:	2005-293T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005293_01

Start Time:	2005-293T00:00	Stop Time:	2005-294T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005294_01

Start Time:	2005-294T00:00	Stop Time:	2005-295T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005295_01

Start Time:	2005-295T00:00	Stop Time:	2005-296T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005296_01

Start Time:	2005-296T00:00	Stop Time:	2005-297T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005297_01

Start Time:	2005-297T00:00	Stop Time:	2005-298T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005298_01

Start Time:	2005-298T00:00	Stop Time:	2005-299T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005299_01

Start Time:	2005-299T00:00	Stop Time:	2005-300T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005300_01

Start Time:	2005-300T00:00	Stop Time:	2005-301T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005301_01

Start Time:	2005-301T00:00	Stop Time:	2005-302T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005302_01

Start Time:	2005-302T00:00	Stop Time:	2005-303T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005303_01

Start Time:	2005-303T00:00	Stop Time:	2005-304T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005304_01

Start Time:	2005-304T00:00	Stop Time:	2005-305T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005305_01

Start Time:	2005-305T00:00	Stop Time:	2005-306T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005306_01

Start Time:	2005-306T00:00	Stop Time:	2005-307T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005307_01

Start Time:	2005-307T00:00	Stop Time:	2005-308T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005308_01

Start Time:	2005-308T00:00	Stop Time:	2005-309T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005309_01

Start Time:	2005-309T00:00	Stop Time:	2005-310T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005310_01

Start Time:	2005-310T00:00	Stop Time:	2005-311T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005311_01

Start Time:	2005-311T00:00	Stop Time:	2005-312T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005312_01

Start Time:	2005-312T00:00	Stop Time:	2005-313T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005313_01

Start Time:	2005-313T00:00	Stop Time:	2005-314T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005314_01

Start Time:	2005-314T00:00	Stop Time:	2005-315T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005315_01

Start Time:	2005-315T00:00	Stop Time:	2005-316T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005316_01

Start Time:	2005-316T00:00	Stop Time:	2005-317T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005317_01

Start Time:	2005-317T00:00	Stop Time:	2005-318T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005318_01

Start Time:	2005-318T00:00	Stop Time:	2005-319T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005319_01

Start Time:	2005-319T00:00	Stop Time:	2005-320T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005320_01

Start Time:	2005-320T00:00	Stop Time:	2005-321T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005321_01

Start Time:	2005-321T00:00	Stop Time:	2005-322T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005322_01

Start Time:	2005-322T00:00	Stop Time:	2005-323T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005323_01

Start Time:	2005-323T00:00	Stop Time:	2005-324T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005324_01

Start Time:	2005-324T00:00	Stop Time:	2005-325T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005325_01

Start Time:	2005-325T00:00	Stop Time:	2005-326T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005326_01

Start Time:	2005-326T00:00	Stop Time:	2005-327T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005327_01

Start Time:	2005-327T00:00	Stop Time:	2005-328T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005328_01

Start Time:	2005-328T00:00	Stop Time:	2005-329T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005329_01

Start Time:	2005-329T00:00	Stop Time:	2005-330T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005330_01

Start Time:	2005-330T00:00	Stop Time:	2005-331T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005331_01

Start Time:	2005-331T00:00	Stop Time:	2005-332T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005332_01

Start Time:	2005-332T00:00	Stop Time:	2005-333T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005333_01

Start Time:	2005-333T00:00	Stop Time:	2005-334T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005334_01

Start Time:	2005-334T00:00	Stop Time:	2005-335T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005335_01

Start Time:	2005-335T00:00	Stop Time:	2005-336T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005336_01

Start Time:	2005-336T00:00	Stop Time:	2005-337T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005337_01

Start Time:	2005-337T00:00	Stop Time:	2005-338T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005338_01

Start Time:	2005-338T00:00	Stop Time:	2005-339T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005339_01

Start Time:	2005-339T00:00	Stop Time:	2005-340T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005340_01

Start Time:	2005-340T00:00	Stop Time:	2005-341T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005341_01

Start Time:	2005-341T00:00	Stop Time:	2005-342T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005342_01

Start Time:	2005-342T00:00	Stop Time:	2005-343T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005343_01

Start Time:	2005-343T00:00	Stop Time:	2005-344T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005344_01

Start Time:	2005-344T00:00	Stop Time:	2005-345T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005345_01

Start Time:	2005-345T00:00	Stop Time:	2005-346T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005346_01

Start Time:	2005-346T00:00	Stop Time:	2005-347T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005347_01

Start Time:	2005-347T00:00	Stop Time:	2005-348T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005348_01

Start Time:	2005-348T00:00	Stop Time:	2005-349T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005349_01

Start Time:	2005-349T00:00	Stop Time:	2005-350T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005350_01

Start Time:	2005-350T00:00	Stop Time:	2005-351T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005351_01

Start Time:	2005-351T00:00	Stop Time:	2005-352T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005352_01

Start Time:	2005-352T00:00	Stop Time:	2005-353T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005353_01

Start Time:	2005-353T00:00	Stop Time:	2005-354T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005354_01

Start Time:	2005-354T00:00	Stop Time:	2005-355T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005355_01

Start Time:	2005-355T00:00	Stop Time:	2005-356T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005356_01

Start Time:	2005-356T00:00	Stop Time:	2005-357T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005357_01

Start Time:	2005-357T00:00	Stop Time:	2005-358T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005358_01

Start Time:	2005-358T00:00	Stop Time:	2005-359T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005359_01

Start Time:	2005-359T00:00	Stop Time:	2005-360T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005360_01

Start Time:	2005-360T00:00	Stop Time:	2005-361T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005361_01

Start Time:	2005-361T00:00	Stop Time:	2005-362T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005362_01

Start Time:	2005-362T00:00	Stop Time:	2005-363T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005363_01

Start Time:	2005-363T00:00	Stop Time:	2005-364T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005364_01

Start Time:	2005-364T00:00	Stop Time:	2005-365T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2005365_01

Start Time:	2005-365T00:00	Stop Time:	2006-001T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the 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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