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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/ 2007 /

LACCAVG0_1MIN_2007002_01

Start Time:	2007-002T00:00	Stop Time:	2007-003T00:00
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_2007003_01

Start Time:	2007-003T00:00	Stop Time:	2007-004T00:00
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_2007004_01

Start Time:	2007-004T00:00	Stop Time:	2007-005T00:00
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_2007005_01

Start Time:	2007-005T00:00	Stop Time:	2007-006T00:00
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_2007006_01

Start Time:	2007-006T00:00	Stop Time:	2007-007T00:00
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_2007007_01

Start Time:	2007-007T00:00	Stop Time:	2007-008T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007008_01

Start Time:	2007-008T00:00	Stop Time:	2007-009T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007009_01

Start Time:	2007-009T00:00	Stop Time:	2007-010T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007010_01

Start Time:	2007-010T00:00	Stop Time:	2007-011T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007011_01

Start Time:	2007-011T00:00	Stop Time:	2007-012T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007012_01

Start Time:	2007-012T00:00	Stop Time:	2007-013T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007013_01

Start Time:	2007-013T00:00	Stop Time:	2007-014T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007014_01

Start Time:	2007-014T00:00	Stop Time:	2007-015T00:00
The data columns contain 1 minute averages of LEMMS accumulator rates data. The data are averaged by first defining fixed one minute intervals throughout the day and then averaging any data points that fall in the intervals. If an interval contains no data, it is still listed in the file, but all data intensity values will be fill. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are four types of channels included in these averages. The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. The file header and leading columns of the file are present to make the format consistent with other MIMI data in the PDS. Note that much of the values for the leading columns are -1, indicating that they do not have useful values, but their presence allows this file to be parsed by the same code that reads other MIMI PDS data. The first column is always the string 'sci', the next column is a UTC string, and then these prefix columns have no data in them but are just there to preserve the format: UTC SCLOCK Start_Ephemeris_s End_Ephemeris_s Spin_Counter Sector Start_Sector_Sclock_major Subsector Microsectors_Covered Spin_Period_s Staring Sensor_Bitrate Just before the data columns are three columns giving the position of the Cassini spacecraft relavtive to Saturn in the SZS frame. The position is given for the middle of the time interval. The units are Saturn radii (60268 km) and the SZS frame is defined as: +Z is Saturn spin axis, +Y is +Z cross the Saturn-Sun line, and +X is +Y cross +Z.

LACCAVG0_1MIN_2007015_01

Start Time:	2007-015T00:00	Stop Time:	2007-016T00:00
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_2007016_01

Start Time:	2007-016T00:00	Stop Time:	2007-017T00:00
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_2007017_01

Start Time:	2007-017T00:00	Stop Time:	2007-018T00:00
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_2007018_01

Start Time:	2007-018T00:00	Stop Time:	2007-019T00:00
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_2007019_01

Start Time:	2007-019T00:00	Stop Time:	2007-020T00:00
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_2007020_01

Start Time:	2007-020T00:00	Stop Time:	2007-021T00:00
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_2007021_01

Start Time:	2007-021T00:00	Stop Time:	2007-022T00:00
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_2007022_01

Start Time:	2007-022T00:00	Stop Time:	2007-023T00:00
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_2007023_01

Start Time:	2007-023T00:00	Stop Time:	2007-024T00:00
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_2007024_01

Start Time:	2007-024T00:00	Stop Time:	2007-025T00:00
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_2007025_01

Start Time:	2007-025T00:00	Stop Time:	2007-026T00:00
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_2007026_01

Start Time:	2007-026T00:00	Stop Time:	2007-027T00:00
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_2007027_01

Start Time:	2007-027T00:00	Stop Time:	2007-028T00:00
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_2007028_01

Start Time:	2007-028T00:00	Stop Time:	2007-029T00:00
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_2007029_01

Start Time:	2007-029T00:00	Stop Time:	2007-030T00:00
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_2007030_01

Start Time:	2007-030T00:00	Stop Time:	2007-031T00:00
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_2007031_01

Start Time:	2007-031T00:00	Stop Time:	2007-032T00:00
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_2007032_01

Start Time:	2007-032T00:00	Stop Time:	2007-033T00:00
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_2007033_01

Start Time:	2007-033T00:00	Stop Time:	2007-034T00:00
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_2007034_01

Start Time:	2007-034T00:00	Stop Time:	2007-035T00:00
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_2007035_01

Start Time:	2007-035T00:00	Stop Time:	2007-036T00:00
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_2007036_01

Start Time:	2007-036T00:00	Stop Time:	2007-037T00:00
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_2007037_01

Start Time:	2007-037T00:00	Stop Time:	2007-038T00:00
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_2007038_01

Start Time:	2007-038T00:00	Stop Time:	2007-039T00:00
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_2007039_01

Start Time:	2007-039T00:00	Stop Time:	2007-040T00:00
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_2007040_01

Start Time:	2007-040T00:00	Stop Time:	2007-041T00:00
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_2007041_01

Start Time:	2007-041T00:00	Stop Time:	2007-042T00:00
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_2007042_01

Start Time:	2007-042T00:00	Stop Time:	2007-043T00:00
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_2007043_01

Start Time:	2007-043T00:00	Stop Time:	2007-044T00:00
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_2007044_01

Start Time:	2007-044T00:00	Stop Time:	2007-045T00:00
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_2007045_01

Start Time:	2007-045T00:00	Stop Time:	2007-046T00:00
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_2007046_01

Start Time:	2007-046T00:00	Stop Time:	2007-047T00:00
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_2007047_01

Start Time:	2007-047T00:00	Stop Time:	2007-048T00:00
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_2007048_01

Start Time:	2007-048T00:00	Stop Time:	2007-049T00:00
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_2007049_01

Start Time:	2007-049T00:00	Stop Time:	2007-050T00:00
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_2007050_01

Start Time:	2007-050T00:00	Stop Time:	2007-051T00:00
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_2007051_01

Start Time:	2007-051T00:00	Stop Time:	2007-052T00:00
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_2007052_01

Start Time:	2007-052T00:00	Stop Time:	2007-053T00:00
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_2007053_01

Start Time:	2007-053T00:00	Stop Time:	2007-054T00:00
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_2007054_01

Start Time:	2007-054T00:00	Stop Time:	2007-055T00:00
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_2007055_01

Start Time:	2007-055T00:00	Stop Time:	2007-056T00:00
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_2007056_01

Start Time:	2007-056T00:00	Stop Time:	2007-057T00:00
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_2007057_01

Start Time:	2007-057T00:00	Stop Time:	2007-058T00:00
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_2007058_01

Start Time:	2007-058T00:00	Stop Time:	2007-059T00:00
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_2007059_01

Start Time:	2007-059T00:00	Stop Time:	2007-060T00:00
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_2007060_01

Start Time:	2007-060T00:00	Stop Time:	2007-061T00:00
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_2007061_01

Start Time:	2007-061T00:00	Stop Time:	2007-062T00:00
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_2007062_01

Start Time:	2007-062T00:00	Stop Time:	2007-063T00:00
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_2007063_01

Start Time:	2007-063T00:00	Stop Time:	2007-064T00:00
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_2007064_01

Start Time:	2007-064T00:00	Stop Time:	2007-065T00:00
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_2007065_01

Start Time:	2007-065T00:00	Stop Time:	2007-066T00:00
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_2007066_01

Start Time:	2007-066T00:00	Stop Time:	2007-067T00:00
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_2007067_01

Start Time:	2007-067T00:00	Stop Time:	2007-068T00:00
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_2007068_01

Start Time:	2007-068T00:00	Stop Time:	2007-069T00:00
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_2007069_01

Start Time:	2007-069T00:00	Stop Time:	2007-070T00:00
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_2007070_01

Start Time:	2007-070T00:00	Stop Time:	2007-071T00:00
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_2007071_01

Start Time:	2007-071T00:00	Stop Time:	2007-072T00:00
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_2007072_01

Start Time:	2007-072T00:00	Stop Time:	2007-073T00:00
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_2007073_01

Start Time:	2007-073T00:00	Stop Time:	2007-074T00:00
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_2007074_01

Start Time:	2007-074T00:00	Stop Time:	2007-075T00:00
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_2007075_01

Start Time:	2007-075T00:00	Stop Time:	2007-076T00:00
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_2007076_01

Start Time:	2007-076T00:00	Stop Time:	2007-077T00:00
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_2007077_01

Start Time:	2007-077T00:00	Stop Time:	2007-078T00:00
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_2007078_01

Start Time:	2007-078T00:00	Stop Time:	2007-079T00:00
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_2007079_01

Start Time:	2007-079T00:00	Stop Time:	2007-080T00:00
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_2007080_01

Start Time:	2007-080T00:00	Stop Time:	2007-081T00:00
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_2007081_01

Start Time:	2007-081T00:00	Stop Time:	2007-082T00:00
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_2007082_01

Start Time:	2007-082T00:00	Stop Time:	2007-083T00:00
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_2007083_01

Start Time:	2007-083T00:00	Stop Time:	2007-084T00:00
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_2007084_01

Start Time:	2007-084T00:00	Stop Time:	2007-085T00:00
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_2007085_01

Start Time:	2007-085T00:00	Stop Time:	2007-086T00:00
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_2007086_01

Start Time:	2007-086T00:00	Stop Time:	2007-087T00:00
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_2007087_01

Start Time:	2007-087T00:00	Stop Time:	2007-088T00:00
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_2007088_01

Start Time:	2007-088T00:00	Stop Time:	2007-089T00:00
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_2007089_01

Start Time:	2007-089T00:00	Stop Time:	2007-090T00:00
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_2007090_01

Start Time:	2007-090T00:00	Stop Time:	2007-091T00:00
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_2007091_01

Start Time:	2007-091T00:00	Stop Time:	2007-092T00:00
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_2007092_01

Start Time:	2007-092T00:00	Stop Time:	2007-093T00:00
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_2007093_01

Start Time:	2007-093T00:00	Stop Time:	2007-094T00:00
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_2007095_01

Start Time:	2007-095T00:00	Stop Time:	2007-096T00:00
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_2007096_01

Start Time:	2007-096T00:00	Stop Time:	2007-097T00:00
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_2007097_01

Start Time:	2007-097T00:00	Stop Time:	2007-098T00:00
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_2007098_01

Start Time:	2007-098T00:00	Stop Time:	2007-099T00:00
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_2007099_01

Start Time:	2007-099T00:00	Stop Time:	2007-100T00:00
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_2007100_01

Start Time:	2007-100T00:00	Stop Time:	2007-101T00:00
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_2007101_01

Start Time:	2007-101T00:00	Stop Time:	2007-102T00:00
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_2007102_01

Start Time:	2007-102T00:00	Stop Time:	2007-103T00:00
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_2007103_01

Start Time:	2007-103T00:00	Stop Time:	2007-104T00:00
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_2007104_01

Start Time:	2007-104T00:00	Stop Time:	2007-105T00:00
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_2007105_01

Start Time:	2007-105T00:00	Stop Time:	2007-106T00:00
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_2007106_01

Start Time:	2007-106T00:00	Stop Time:	2007-107T00:00
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_2007107_01

Start Time:	2007-107T00:00	Stop Time:	2007-108T00:00
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_2007108_01

Start Time:	2007-108T00:00	Stop Time:	2007-109T00:00
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_2007109_01

Start Time:	2007-109T00:00	Stop Time:	2007-110T00:00
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_2007110_01

Start Time:	2007-110T00:00	Stop Time:	2007-111T00:00
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_2007111_01

Start Time:	2007-111T00:00	Stop Time:	2007-112T00:00
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_2007112_01

Start Time:	2007-112T00:00	Stop Time:	2007-113T00:00
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_2007113_01

Start Time:	2007-113T00:00	Stop Time:	2007-114T00:00
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_2007114_01

Start Time:	2007-114T00:00	Stop Time:	2007-115T00:00
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_2007115_01

Start Time:	2007-115T00:00	Stop Time:	2007-116T00:00
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_2007116_01

Start Time:	2007-116T00:00	Stop Time:	2007-117T00:00
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_2007117_01

Start Time:	2007-117T00:00	Stop Time:	2007-118T00:00
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_2007118_01

Start Time:	2007-118T00:00	Stop Time:	2007-119T00:00
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_2007119_01

Start Time:	2007-119T00:00	Stop Time:	2007-120T00:00
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_2007120_01

Start Time:	2007-120T00:00	Stop Time:	2007-121T00:00
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_2007121_01

Start Time:	2007-121T00:00	Stop Time:	2007-122T00:00
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_2007122_01

Start Time:	2007-122T00:00	Stop Time:	2007-123T00:00
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_2007123_01

Start Time:	2007-123T00:00	Stop Time:	2007-124T00:00
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_2007124_01

Start Time:	2007-124T00:00	Stop Time:	2007-125T00:00
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_2007125_01

Start Time:	2007-125T00:00	Stop Time:	2007-126T00:00
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_2007126_01

Start Time:	2007-126T00:00	Stop Time:	2007-127T00:00
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_2007127_01

Start Time:	2007-127T00:00	Stop Time:	2007-128T00:00
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_2007128_01

Start Time:	2007-128T00:00	Stop Time:	2007-129T00:00
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_2007129_01

Start Time:	2007-129T00:00	Stop Time:	2007-130T00:00
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_2007130_01

Start Time:	2007-130T00:00	Stop Time:	2007-131T00:00
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_2007131_01

Start Time:	2007-131T00:00	Stop Time:	2007-132T00:00
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_2007132_01

Start Time:	2007-132T00:00	Stop Time:	2007-133T00:00
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_2007133_01

Start Time:	2007-133T00:00	Stop Time:	2007-134T00:00
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_2007134_01

Start Time:	2007-134T00:00	Stop Time:	2007-135T00:00
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_2007135_01

Start Time:	2007-135T00:00	Stop Time:	2007-136T00:00
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_2007136_01

Start Time:	2007-136T00:00	Stop Time:	2007-137T00:00
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_2007137_01

Start Time:	2007-137T00:00	Stop Time:	2007-138T00:00
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_2007138_01

Start Time:	2007-138T00:00	Stop Time:	2007-139T00:00
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_2007139_01

Start Time:	2007-139T00:00	Stop Time:	2007-140T00:00
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_2007140_01

Start Time:	2007-140T00:00	Stop Time:	2007-141T00:00
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_2007141_01

Start Time:	2007-141T00:00	Stop Time:	2007-142T00:00
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_2007142_01

Start Time:	2007-142T00:00	Stop Time:	2007-143T00:00
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_2007143_01

Start Time:	2007-143T00:00	Stop Time:	2007-144T00:00
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_2007144_01

Start Time:	2007-144T00:00	Stop Time:	2007-145T00:00
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_2007145_01

Start Time:	2007-145T00:00	Stop Time:	2007-146T00:00
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_2007146_01

Start Time:	2007-146T00:00	Stop Time:	2007-147T00:00
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_2007147_01

Start Time:	2007-147T00:00	Stop Time:	2007-148T00:00
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_2007148_01

Start Time:	2007-148T00:00	Stop Time:	2007-149T00:00
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_2007149_01

Start Time:	2007-149T00:00	Stop Time:	2007-150T00:00
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_2007150_01

Start Time:	2007-150T00:00	Stop Time:	2007-151T00:00
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_2007151_01

Start Time:	2007-151T00:00	Stop Time:	2007-152T00:00
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_2007152_01

Start Time:	2007-152T00:00	Stop Time:	2007-153T00:00
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_2007153_01

Start Time:	2007-153T00:00	Stop Time:	2007-154T00:00
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_2007154_01

Start Time:	2007-154T00:00	Stop Time:	2007-155T00:00
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_2007155_01

Start Time:	2007-155T00:00	Stop Time:	2007-156T00:00
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_2007156_01

Start Time:	2007-156T00:00	Stop Time:	2007-157T00:00
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_2007157_01

Start Time:	2007-157T00:00	Stop Time:	2007-158T00:00
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_2007158_01

Start Time:	2007-158T00:00	Stop Time:	2007-159T00:00
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_2007159_01

Start Time:	2007-159T00:00	Stop Time:	2007-160T00:00
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_2007160_01

Start Time:	2007-160T00:00	Stop Time:	2007-161T00:00
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_2007161_01

Start Time:	2007-161T00:00	Stop Time:	2007-162T00:00
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_2007162_01

Start Time:	2007-162T00:00	Stop Time:	2007-163T00:00
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_2007163_01

Start Time:	2007-163T00:00	Stop Time:	2007-164T00:00
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_2007164_01

Start Time:	2007-164T00:00	Stop Time:	2007-165T00:00
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_2007165_01

Start Time:	2007-165T00:00	Stop Time:	2007-166T00:00
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_2007166_01

Start Time:	2007-166T00:00	Stop Time:	2007-167T00:00
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_2007167_01

Start Time:	2007-167T00:00	Stop Time:	2007-168T00:00
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_2007168_01

Start Time:	2007-168T00:00	Stop Time:	2007-169T00:00
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_2007169_01

Start Time:	2007-169T00:00	Stop Time:	2007-170T00:00
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_2007170_01

Start Time:	2007-170T00:00	Stop Time:	2007-171T00:00
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_2007171_01

Start Time:	2007-171T00:00	Stop Time:	2007-172T00:00
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_2007172_01

Start Time:	2007-172T00:00	Stop Time:	2007-173T00:00
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_2007173_01

Start Time:	2007-173T00:00	Stop Time:	2007-174T00:00
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_2007174_01

Start Time:	2007-174T00:00	Stop Time:	2007-175T00:00
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_2007175_01

Start Time:	2007-175T00:00	Stop Time:	2007-176T00:00
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_2007176_01

Start Time:	2007-176T00:00	Stop Time:	2007-177T00:00
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_2007177_01

Start Time:	2007-177T00:00	Stop Time:	2007-178T00:00
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_2007178_01

Start Time:	2007-178T00:00	Stop Time:	2007-179T00:00
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_2007179_01

Start Time:	2007-179T00:00	Stop Time:	2007-180T00:00
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_2007180_01

Start Time:	2007-180T00:00	Stop Time:	2007-181T00:00
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_2007181_01

Start Time:	2007-181T00:00	Stop Time:	2007-182T00:00
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_2007182_01

Start Time:	2007-182T00:00	Stop Time:	2007-183T00:00
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_2007183_01

Start Time:	2007-183T00:00	Stop Time:	2007-184T00:00
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_2007184_01

Start Time:	2007-184T00:00	Stop Time:	2007-185T00:00
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_2007185_01

Start Time:	2007-185T00:00	Stop Time:	2007-186T00:00
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_2007186_01

Start Time:	2007-186T00:00	Stop Time:	2007-187T00:00
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_2007187_01

Start Time:	2007-187T00:00	Stop Time:	2007-188T00:00
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_2007188_01

Start Time:	2007-188T00:00	Stop Time:	2007-189T00:00
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_2007189_01

Start Time:	2007-189T00:00	Stop Time:	2007-190T00:00
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_2007190_01

Start Time:	2007-190T00:00	Stop Time:	2007-191T00:00
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_2007191_01

Start Time:	2007-191T00:00	Stop Time:	2007-192T00:00
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_2007192_01

Start Time:	2007-192T00:00	Stop Time:	2007-193T00:00
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_2007193_01

Start Time:	2007-193T00:00	Stop Time:	2007-194T00:00
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_2007194_01

Start Time:	2007-194T00:00	Stop Time:	2007-195T00:00
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_2007195_01

Start Time:	2007-195T00:00	Stop Time:	2007-196T00:00
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_2007196_01

Start Time:	2007-196T00:00	Stop Time:	2007-197T00:00
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_2007197_01

Start Time:	2007-197T00:00	Stop Time:	2007-198T00:00
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_2007198_01

Start Time:	2007-198T00:00	Stop Time:	2007-199T00:00
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_2007199_01

Start Time:	2007-199T00:00	Stop Time:	2007-200T00:00
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_2007200_01

Start Time:	2007-200T00:00	Stop Time:	2007-201T00:00
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_2007201_01

Start Time:	2007-201T00:00	Stop Time:	2007-202T00:00
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_2007202_01

Start Time:	2007-202T00:00	Stop Time:	2007-203T00:00
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_2007203_01

Start Time:	2007-203T00:00	Stop Time:	2007-204T00:00
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_2007204_01

Start Time:	2007-204T00:00	Stop Time:	2007-205T00:00
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_2007205_01

Start Time:	2007-205T00:00	Stop Time:	2007-206T00:00
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_2007206_01

Start Time:	2007-206T00:00	Stop Time:	2007-207T00:00
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_2007207_01

Start Time:	2007-207T00:00	Stop Time:	2007-208T00:00
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_2007208_01

Start Time:	2007-208T00:00	Stop Time:	2007-209T00:00
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_2007209_01

Start Time:	2007-209T00:00	Stop Time:	2007-210T00:00
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_2007210_01

Start Time:	2007-210T00:00	Stop Time:	2007-211T00:00
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_2007211_01

Start Time:	2007-211T00:00	Stop Time:	2007-212T00:00
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_2007212_01

Start Time:	2007-212T00:00	Stop Time:	2007-213T00:00
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_2007213_01

Start Time:	2007-213T00:00	Stop Time:	2007-214T00:00
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_2007214_01

Start Time:	2007-214T00:00	Stop Time:	2007-215T00:00
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_2007215_01

Start Time:	2007-215T00:00	Stop Time:	2007-216T00:00
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_2007216_01

Start Time:	2007-216T00:00	Stop Time:	2007-217T00:00
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_2007217_01

Start Time:	2007-217T00:00	Stop Time:	2007-218T00:00
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_2007218_01

Start Time:	2007-218T00:00	Stop Time:	2007-219T00:00
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_2007219_01

Start Time:	2007-219T00:00	Stop Time:	2007-220T00:00
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_2007220_01

Start Time:	2007-220T00:00	Stop Time:	2007-221T00:00
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_2007221_01

Start Time:	2007-221T00:00	Stop Time:	2007-222T00:00
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_2007222_01

Start Time:	2007-222T00:00	Stop Time:	2007-223T00:00
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_2007223_01

Start Time:	2007-223T00:00	Stop Time:	2007-224T00:00
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_2007224_01

Start Time:	2007-224T00:00	Stop Time:	2007-225T00:00
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_2007225_01

Start Time:	2007-225T00:00	Stop Time:	2007-226T00:00
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_2007226_01

Start Time:	2007-226T00:00	Stop Time:	2007-227T00:00
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_2007227_01

Start Time:	2007-227T00:00	Stop Time:	2007-228T00:00
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_2007228_01

Start Time:	2007-228T00:00	Stop Time:	2007-229T00:00
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_2007229_01

Start Time:	2007-229T00:00	Stop Time:	2007-230T00:00
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_2007230_01

Start Time:	2007-230T00:00	Stop Time:	2007-231T00:00
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_2007231_01

Start Time:	2007-231T00:00	Stop Time:	2007-232T00:00
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_2007232_01

Start Time:	2007-232T00:00	Stop Time:	2007-233T00:00
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_2007233_01

Start Time:	2007-233T00:00	Stop Time:	2007-234T00:00
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_2007234_01

Start Time:	2007-234T00:00	Stop Time:	2007-235T00:00
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_2007235_01

Start Time:	2007-235T00:00	Stop Time:	2007-236T00:00
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_2007236_01

Start Time:	2007-236T00:00	Stop Time:	2007-237T00:00
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_2007237_01

Start Time:	2007-237T00:00	Stop Time:	2007-238T00:00
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_2007238_01

Start Time:	2007-238T00:00	Stop Time:	2007-239T00:00
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_2007239_01

Start Time:	2007-239T00:00	Stop Time:	2007-240T00:00
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_2007240_01

Start Time:	2007-240T00:00	Stop Time:	2007-241T00:00
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_2007241_01

Start Time:	2007-241T00:00	Stop Time:	2007-242T00:00
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_2007242_01

Start Time:	2007-242T00:00	Stop Time:	2007-243T00:00
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_2007243_01

Start Time:	2007-243T00:00	Stop Time:	2007-244T00:00
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_2007244_01

Start Time:	2007-244T00:00	Stop Time:	2007-245T00:00
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_2007245_01

Start Time:	2007-245T00:00	Stop Time:	2007-246T00:00
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_2007246_01

Start Time:	2007-246T00:00	Stop Time:	2007-247T00:00
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_2007247_01

Start Time:	2007-247T00:00	Stop Time:	2007-248T00:00
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_2007248_01

Start Time:	2007-248T00:00	Stop Time:	2007-249T00:00
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_2007249_01

Start Time:	2007-249T00:00	Stop Time:	2007-250T00:00
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_2007250_01

Start Time:	2007-250T00:00	Stop Time:	2007-251T00:00
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_2007251_01

Start Time:	2007-251T00:00	Stop Time:	2007-252T00:00
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_2007252_01

Start Time:	2007-252T00:00	Stop Time:	2007-253T00:00
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_2007253_01

Start Time:	2007-253T00:00	Stop Time:	2007-254T00:00
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_2007254_01

Start Time:	2007-254T00:00	Stop Time:	2007-255T00:00
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_2007258_01

Start Time:	2007-258T00:00	Stop Time:	2007-259T00:00
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_2007259_01

Start Time:	2007-259T00:00	Stop Time:	2007-260T00:00
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_2007260_01

Start Time:	2007-260T00:00	Stop Time:	2007-261T00:00
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_2007261_01

Start Time:	2007-261T00:00	Stop Time:	2007-262T00:00
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_2007262_01

Start Time:	2007-262T00:00	Stop Time:	2007-263T00:00
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_2007263_01

Start Time:	2007-263T00:00	Stop Time:	2007-264T00:00
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_2007264_01

Start Time:	2007-264T00:00	Stop Time:	2007-265T00:00
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_2007265_01

Start Time:	2007-265T00:00	Stop Time:	2007-266T00:00
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_2007266_01

Start Time:	2007-266T00:00	Stop Time:	2007-267T00:00
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_2007267_01

Start Time:	2007-267T00:00	Stop Time:	2007-268T00:00
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_2007268_01

Start Time:	2007-268T00:00	Stop Time:	2007-269T00:00
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_2007269_01

Start Time:	2007-269T00:00	Stop Time:	2007-270T00:00
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_2007270_01

Start Time:	2007-270T00:00	Stop Time:	2007-271T00:00
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_2007271_01

Start Time:	2007-271T00:00	Stop Time:	2007-272T00:00
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_2007272_01

Start Time:	2007-272T00:00	Stop Time:	2007-273T00:00
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_2007273_01

Start Time:	2007-273T00:00	Stop Time:	2007-274T00:00
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_2007274_01

Start Time:	2007-274T00:00	Stop Time:	2007-275T00:00
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_2007275_01

Start Time:	2007-275T00:00	Stop Time:	2007-276T00:00
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_2007276_01

Start Time:	2007-276T00:00	Stop Time:	2007-277T00:00
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_2007277_01

Start Time:	2007-277T00:00	Stop Time:	2007-278T00:00
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_2007278_01

Start Time:	2007-278T00:00	Stop Time:	2007-279T00:00
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_2007279_01

Start Time:	2007-279T00:00	Stop Time:	2007-280T00:00
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_2007291_01

Start Time:	2007-291T00:00	Stop Time:	2007-292T00:00
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_2007292_01

Start Time:	2007-292T00:00	Stop Time:	2007-293T00:00
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_2007293_01

Start Time:	2007-293T00:00	Stop Time:	2007-294T00:00
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_2007294_01

Start Time:	2007-294T00:00	Stop Time:	2007-295T00:00
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_2007295_01

Start Time:	2007-295T00:00	Stop Time:	2007-296T00:00
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_2007296_01

Start Time:	2007-296T00:00	Stop Time:	2007-297T00:00
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_2007297_01

Start Time:	2007-297T00:00	Stop Time:	2007-298T00:00
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_2007298_01

Start Time:	2007-298T00:00	Stop Time:	2007-299T00:00
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_2007299_01

Start Time:	2007-299T00:00	Stop Time:	2007-300T00:00
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_2007300_01

Start Time:	2007-300T00:00	Stop Time:	2007-301T00:00
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_2007301_01

Start Time:	2007-301T00:00	Stop Time:	2007-302T00:00
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_2007302_01

Start Time:	2007-302T00:00	Stop Time:	2007-303T00:00
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_2007303_01

Start Time:	2007-303T00:00	Stop Time:	2007-304T00:00
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_2007304_01

Start Time:	2007-304T00:00	Stop Time:	2007-305T00:00
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_2007305_01

Start Time:	2007-305T00:00	Stop Time:	2007-306T00:00
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_2007306_01

Start Time:	2007-306T00:00	Stop Time:	2007-307T00:00
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_2007307_01

Start Time:	2007-307T00:00	Stop Time:	2007-308T00:00
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_2007308_01

Start Time:	2007-308T00:00	Stop Time:	2007-309T00:00
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_2007309_01

Start Time:	2007-309T00:00	Stop Time:	2007-310T00:00
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_2007310_01

Start Time:	2007-310T00:00	Stop Time:	2007-311T00:00
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_2007311_01

Start Time:	2007-311T00:00	Stop Time:	2007-312T00:00
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_2007312_01

Start Time:	2007-312T00:00	Stop Time:	2007-313T00:00
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_2007313_01

Start Time:	2007-313T00:00	Stop Time:	2007-314T00:00
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_2007314_01

Start Time:	2007-314T00:00	Stop Time:	2007-315T00:00
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_2007315_01

Start Time:	2007-315T00:00	Stop Time:	2007-316T00:00
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_2007316_01

Start Time:	2007-316T00:00	Stop Time:	2007-317T00:00
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_2007317_01

Start Time:	2007-317T00:00	Stop Time:	2007-318T00:00
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_2007318_01

Start Time:	2007-318T00:00	Stop Time:	2007-319T00:00
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_2007319_01

Start Time:	2007-319T00:00	Stop Time:	2007-320T00:00
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_2007320_01

Start Time:	2007-320T00:00	Stop Time:	2007-321T00:00
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_2007321_01

Start Time:	2007-321T00:00	Stop Time:	2007-322T00:00
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_2007322_01

Start Time:	2007-322T00:00	Stop Time:	2007-323T00:00
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_2007323_01

Start Time:	2007-323T00:00	Stop Time:	2007-324T00:00
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_2007324_01

Start Time:	2007-324T00:00	Stop Time:	2007-325T00:00
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_2007325_01

Start Time:	2007-325T00:00	Stop Time:	2007-326T00:00
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_2007326_01

Start Time:	2007-326T00:00	Stop Time:	2007-327T00:00
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_2007327_01

Start Time:	2007-327T00:00	Stop Time:	2007-328T00:00
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_2007328_01

Start Time:	2007-328T00:00	Stop Time:	2007-329T00:00
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_2007329_01

Start Time:	2007-329T00:00	Stop Time:	2007-330T00:00
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_2007330_01

Start Time:	2007-330T00:00	Stop Time:	2007-331T00:00
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_2007331_01

Start Time:	2007-331T00:00	Stop Time:	2007-332T00:00
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_2007332_01

Start Time:	2007-332T00:00	Stop Time:	2007-333T00:00
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_2007333_01

Start Time:	2007-333T00:00	Stop Time:	2007-334T00:00
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_2007334_01

Start Time:	2007-334T00:00	Stop Time:	2007-335T00:00
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_2007335_01

Start Time:	2007-335T00:00	Stop Time:	2007-336T00:00
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_2007336_01

Start Time:	2007-336T00:00	Stop Time:	2007-337T00:00
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_2007337_01

Start Time:	2007-337T00:00	Stop Time:	2007-338T00:00
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_2007338_01

Start Time:	2007-338T00:00	Stop Time:	2007-339T00:00
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_2007339_01

Start Time:	2007-339T00:00	Stop Time:	2007-340T00:00
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_2007340_01

Start Time:	2007-340T00:00	Stop Time:	2007-341T00:00
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_2007341_01

Start Time:	2007-341T00:00	Stop Time:	2007-342T00:00
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_2007342_01

Start Time:	2007-342T00:00	Stop Time:	2007-343T00:00
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_2007343_01

Start Time:	2007-343T00:00	Stop Time:	2007-344T00:00
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_2007344_01

Start Time:	2007-344T00:00	Stop Time:	2007-345T00:00
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_2007345_01

Start Time:	2007-345T00:00	Stop Time:	2007-346T00:00
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_2007346_01

Start Time:	2007-346T00:00	Stop Time:	2007-347T00:00
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_2007347_01

Start Time:	2007-347T00:00	Stop Time:	2007-348T00:00
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_2007348_01

Start Time:	2007-348T00:00	Stop Time:	2007-349T00:00
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_2007349_01

Start Time:	2007-349T00:00	Stop Time:	2007-350T00:00
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_2007350_01

Start Time:	2007-350T00:00	Stop Time:	2007-351T00:00
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_2007351_01

Start Time:	2007-351T00:00	Stop Time:	2007-352T00:00
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_2007352_01

Start Time:	2007-352T00:00	Stop Time:	2007-353T00:00
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_2007353_01

Start Time:	2007-353T00:00	Stop Time:	2007-354T00:00
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_2007354_01

Start Time:	2007-354T00:00	Stop Time:	2007-355T00:00
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_2007355_01

Start Time:	2007-355T00:00	Stop Time:	2007-356T00:00
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_2007356_01

Start Time:	2007-356T00:00	Stop Time:	2007-357T00:00
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_2007357_01

Start Time:	2007-357T00:00	Stop Time:	2007-358T00:00
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_2007358_01

Start Time:	2007-358T00:00	Stop Time:	2007-359T00:00
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_2007359_01

Start Time:	2007-359T00:00	Stop Time:	2007-360T00:00
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_2007360_01

Start Time:	2007-360T00:00	Stop Time:	2007-361T00:00
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_2007361_01

Start Time:	2007-361T00:00	Stop Time:	2007-362T00:00
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_2007362_01

Start Time:	2007-362T00:00	Stop Time:	2007-363T00:00
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_2007363_01

Start Time:	2007-363T00:00	Stop Time:	2007-364T00:00
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_2007364_01

Start Time:	2007-364T00:00	Stop Time:	2007-365T00:00
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_2007365_01

Start Time:	2007-365T00:00	Stop Time:	2008-001T00:00
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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