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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/ LACCFULL0/ 2007 /

LACCFULL0_2007001_01

Start Time:	2007-001T00:00:00.922	Stop Time:	2007-001T23:59:58.624
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007002_01

Start Time:	2007-002T00:00:02.374	Stop Time:	2007-002T23:59:56.743
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007003_01

Start Time:	2007-003T00:00:03.079	Stop Time:	2007-003T23:59:58.530
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007004_01

Start Time:	2007-004T00:00:02.276	Stop Time:	2007-004T23:59:58.228
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007005_01

Start Time:	2007-005T00:00:01.978	Stop Time:	2007-005T23:59:57.804
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007006_01

Start Time:	2007-006T00:00:02.491	Stop Time:	2007-006T23:59:54.400
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007007_01

Start Time:	2007-007T00:00:00.884	Stop Time:	2007-007T23:59:57.832
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007008_01

Start Time:	2007-008T00:00:01.582	Stop Time:	2007-008T23:59:57.658
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007009_01

Start Time:	2007-009T00:00:03.283	Stop Time:	2007-009T23:59:56.234
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007010_01

Start Time:	2007-010T00:00:01.859	Stop Time:	2007-010T23:59:55.435
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007011_01

Start Time:	2007-011T00:00:01.060	Stop Time:	2007-011T23:59:58.137
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007012_01

Start Time:	2007-012T00:00:03.762	Stop Time:	2007-012T23:59:57.838
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007013_01

Start Time:	2007-013T00:00:03.463	Stop Time:	2007-013T23:59:59.289
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007014_01

Start Time:	2007-014T00:00:04.914	Stop Time:	2007-014T23:59:57.866
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007015_01

Start Time:	2007-015T00:00:02.553	Stop Time:	2007-015T23:59:56.692
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007016_01

Start Time:	2007-016T00:00:00.442	Stop Time:	2007-016T23:59:58.143
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007017_01

Start Time:	2007-017T00:00:01.893	Stop Time:	2007-017T23:59:58.532
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007018_01

Start Time:	2007-018T00:00:01.345	Stop Time:	2007-018T23:59:56.546
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007019_01

Start Time:	2007-019T00:00:00.296	Stop Time:	2007-019T23:59:57.247
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007020_01

Start Time:	2007-020T00:00:00.997	Stop Time:	2007-020T23:59:59.949
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007021_01

Start Time:	2007-021T00:00:03.698	Stop Time:	2007-021T23:59:57.653
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007022_01

Start Time:	2007-022T00:00:01.399	Stop Time:	2007-022T23:59:59.100
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007023_01

Start Time:	2007-023T00:00:02.850	Stop Time:	2007-023T23:59:54.770
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007024_01

Start Time:	2007-024T00:00:01.071	Stop Time:	2007-024T23:59:59.378
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007025_01

Start Time:	2007-025T00:00:05.007	Stop Time:	2007-025T23:59:57.847
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007026_01

Start Time:	2007-026T00:00:03.472	Stop Time:	2007-026T23:59:55.426
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007027_01

Start Time:	2007-027T00:00:01.051	Stop Time:	2007-027T23:59:59.879
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007028_01

Start Time:	2007-028T00:00:05.504	Stop Time:	2007-028T23:59:54.832
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007029_01

Start Time:	2007-029T00:00:00.457	Stop Time:	2007-029T23:59:55.289
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007030_01

Start Time:	2007-030T00:00:00.910	Stop Time:	2007-030T23:59:56.739
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007031_01

Start Time:	2007-031T00:00:00.489	Stop Time:	2007-031T23:59:59.192
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007032_01

Start Time:	2007-032T00:00:02.942	Stop Time:	2007-032T23:59:56.895
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007033_01

Start Time:	2007-033T00:00:00.645	Stop Time:	2007-033T23:59:57.837
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007034_01

Start Time:	2007-034T00:00:04.177	Stop Time:	2007-034T23:59:57.614
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007035_01

Start Time:	2007-035T00:00:00.427	Stop Time:	2007-035T23:59:58.130
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007036_01

Start Time:	2007-036T00:00:02.818	Stop Time:	2007-036T23:59:56.708
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007037_01

Start Time:	2007-037T00:00:00.458	Stop Time:	2007-037T23:59:58.162
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007038_01

Start Time:	2007-038T00:00:01.912	Stop Time:	2007-038T23:59:59.615
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007039_01

Start Time:	2007-039T00:00:03.365	Stop Time:	2007-039T23:59:57.971
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007040_01

Start Time:	2007-040T00:00:04.330	Stop Time:	2007-040T23:59:59.275
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007041_01

Start Time:	2007-041T00:00:03.022	Stop Time:	2007-041T23:59:59.850
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007042_01

Start Time:	2007-042T00:00:02.662	Stop Time:	2007-042T23:59:57.678
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007043_01

Start Time:	2007-043T00:00:00.491	Stop Time:	2007-043T23:59:58.081
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007044_01

Start Time:	2007-044T00:00:04.420	Stop Time:	2007-044T21:45:21.323
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007045_01

Start Time:	2007-045T00:18:14.410	Stop Time:	2007-045T23:59:58.913
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007046_01

Start Time:	2007-046T00:00:04.542	Stop Time:	2007-046T23:59:55.655
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007047_01

Start Time:	2007-047T00:00:06.839	Stop Time:	2007-047T23:59:59.820
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007048_01

Start Time:	2007-048T00:00:02.632	Stop Time:	2007-048T23:59:58.398
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007049_01

Start Time:	2007-049T00:00:02.148	Stop Time:	2007-049T23:59:59.101
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007050_01

Start Time:	2007-050T00:00:02.851	Stop Time:	2007-050T23:59:56.804
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007051_01

Start Time:	2007-051T00:00:00.554	Stop Time:	2007-051T19:22:37.613
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007052_01

Start Time:	2007-052T00:10:42.257	Stop Time:	2007-052T10:39:53.265
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007053_01

Start Time:	2007-053T02:42:15.653	Stop Time:	2007-053T12:59:22.790
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007054_01

Start Time:	2007-054T00:59:31.145	Stop Time:	2007-054T23:59:58.867
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007055_01

Start Time:	2007-055T00:00:02.617	Stop Time:	2007-055T23:59:58.071
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007056_01

Start Time:	2007-056T00:00:01.821	Stop Time:	2007-056T23:59:59.524
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007057_01

Start Time:	2007-057T00:00:03.274	Stop Time:	2007-057T23:59:57.227
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007058_01

Start Time:	2007-058T00:00:00.977	Stop Time:	2007-058T23:59:58.181
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007059_01

Start Time:	2007-059T00:00:01.931	Stop Time:	2007-059T23:59:57.134
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007060_01

Start Time:	2007-060T00:00:00.888	Stop Time:	2007-060T23:59:57.087
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007061_01

Start Time:	2007-061T00:00:00.837	Stop Time:	2007-061T23:59:58.915
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007062_01

Start Time:	2007-062T00:00:04.540	Stop Time:	2007-062T23:59:58.119
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007063_01

Start Time:	2007-063T00:00:03.744	Stop Time:	2007-063T23:59:59.045
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007064_01

Start Time:	2007-064T00:00:05.314	Stop Time:	2007-064T23:59:54.822
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007065_01

Start Time:	2007-065T00:00:01.158	Stop Time:	2007-065T23:59:57.103
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007066_01

Start Time:	2007-066T00:00:01.791	Stop Time:	2007-066T23:59:58.557
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007067_01

Start Time:	2007-067T00:00:02.307	Stop Time:	2007-067T23:59:59.760
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007068_01

Start Time:	2007-068T00:00:03.510	Stop Time:	2007-068T23:59:59.087
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007069_01

Start Time:	2007-069T00:00:01.900	Stop Time:	2007-069T23:59:58.982
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007070_01

Start Time:	2007-070T00:00:05.267	Stop Time:	2007-070T23:59:58.931
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007071_01

Start Time:	2007-071T00:00:01.744	Stop Time:	2007-071T23:59:58.072
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007072_01

Start Time:	2007-072T00:00:00.885	Stop Time:	2007-072T23:59:58.713
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007073_01

Start Time:	2007-073T00:00:01.525	Stop Time:	2007-073T23:59:58.354
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007074_01

Start Time:	2007-074T00:00:01.166	Stop Time:	2007-074T23:59:57.369
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007075_01

Start Time:	2007-075T00:00:00.182	Stop Time:	2007-075T23:59:58.635
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007076_01

Start Time:	2007-076T00:00:01.448	Stop Time:	2007-076T23:59:58.276
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007077_01

Start Time:	2007-077T00:00:01.088	Stop Time:	2007-077T23:59:58.917
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007078_01

Start Time:	2007-078T00:00:01.729	Stop Time:	2007-078T23:59:59.370
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007079_01

Start Time:	2007-079T00:00:04.995	Stop Time:	2007-079T23:59:54.823
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007080_01

Start Time:	2007-080T00:00:00.448	Stop Time:	2007-080T23:59:58.276
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007081_01

Start Time:	2007-081T00:00:03.901	Stop Time:	2007-081T23:59:55.230
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007082_01

Start Time:	2007-082T00:00:00.859	Stop Time:	2007-082T23:59:57.558
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007083_01

Start Time:	2007-083T00:00:01.312	Stop Time:	2007-083T23:59:56.867
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007084_01

Start Time:	2007-084T00:00:03.210	Stop Time:	2007-084T23:59:58.089
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007085_01

Start Time:	2007-085T00:00:00.902	Stop Time:	2007-085T23:59:58.730
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007086_01

Start Time:	2007-086T00:00:01.543	Stop Time:	2007-086T23:59:58.371
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007087_01

Start Time:	2007-087T00:00:01.183	Stop Time:	2007-087T23:59:59.012
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007088_01

Start Time:	2007-088T00:00:01.824	Stop Time:	2007-088T23:59:58.653
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007089_01

Start Time:	2007-089T00:00:01.465	Stop Time:	2007-089T23:59:59.903
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007090_01

Start Time:	2007-090T00:00:06.242	Stop Time:	2007-090T23:59:58.372
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007091_01

Start Time:	2007-091T00:00:01.184	Stop Time:	2007-091T23:59:58.012
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007092_01

Start Time:	2007-092T00:00:00.825	Stop Time:	2007-092T23:59:58.653
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007093_01

Start Time:	2007-093T00:00:01.466	Stop Time:	2007-093T23:14:37.561
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007095_01

Start Time:	2007-095T03:57:48.661	Stop Time:	2007-095T23:59:59.450
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007096_01

Start Time:	2007-096T00:00:03.204	Stop Time:	2007-096T23:59:59.029
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007097_01

Start Time:	2007-097T00:00:01.841	Stop Time:	2007-097T23:59:59.669
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007098_01

Start Time:	2007-098T00:00:02.482	Stop Time:	2007-098T23:59:57.748
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007099_01

Start Time:	2007-099T00:00:02.435	Stop Time:	2007-099T23:59:58.263
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007100_01

Start Time:	2007-100T00:00:02.951	Stop Time:	2007-100T23:59:59.320
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007101_01

Start Time:	2007-101T00:00:04.945	Stop Time:	2007-101T23:59:55.214
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007102_01

Start Time:	2007-102T00:00:01.515	Stop Time:	2007-102T23:59:59.850
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007103_01

Start Time:	2007-103T00:00:02.663	Stop Time:	2007-103T23:59:58.991
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007104_01

Start Time:	2007-104T00:00:01.807	Stop Time:	2007-104T23:59:59.631
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007105_01

Start Time:	2007-105T00:00:02.444	Stop Time:	2007-105T23:59:59.272
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007106_01

Start Time:	2007-106T00:00:02.084	Stop Time:	2007-106T23:59:57.998
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007107_01

Start Time:	2007-107T00:00:04.365	Stop Time:	2007-107T23:59:57.803
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007108_01

Start Time:	2007-108T00:00:00.619	Stop Time:	2007-108T23:59:58.443
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007109_01

Start Time:	2007-109T00:00:01.255	Stop Time:	2007-109T23:59:58.083
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007110_01

Start Time:	2007-110T00:00:00.896	Stop Time:	2007-110T23:59:55.614
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007111_01

Start Time:	2007-111T00:00:01.907	Stop Time:	2007-111T23:59:54.970
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007112_01

Start Time:	2007-112T00:00:01.286	Stop Time:	2007-112T23:59:54.692
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007113_01

Start Time:	2007-113T00:00:01.008	Stop Time:	2007-113T23:59:56.266
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007114_01

Start Time:	2007-114T00:00:02.590	Stop Time:	2007-114T23:59:57.535
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007115_01

Start Time:	2007-115T00:00:01.285	Stop Time:	2007-115T23:59:58.758
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007116_01

Start Time:	2007-116T00:00:05.242	Stop Time:	2007-116T23:59:56.441
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007117_01

Start Time:	2007-117T00:00:02.066	Stop Time:	2007-117T23:59:57.707
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007118_01

Start Time:	2007-118T00:00:00.519	Stop Time:	2007-118T23:59:56.406
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007119_01

Start Time:	2007-119T00:00:02.706	Stop Time:	2007-119T23:59:57.801
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007120_01

Start Time:	2007-120T00:00:00.613	Stop Time:	2007-120T23:59:58.441
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007121_01

Start Time:	2007-121T00:00:01.254	Stop Time:	2007-121T23:33:11.154
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007122_01

Start Time:	2007-122T12:09:16.683	Stop Time:	2007-122T23:59:58.660
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007123_01

Start Time:	2007-123T00:00:01.472	Stop Time:	2007-123T23:59:54.269
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007124_01

Start Time:	2007-124T00:00:00.577	Stop Time:	2007-124T23:59:58.378
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007125_01

Start Time:	2007-125T00:00:01.190	Stop Time:	2007-125T23:59:59.018
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007126_01

Start Time:	2007-126T00:00:01.831	Stop Time:	2007-126T23:59:58.659
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007127_01

Start Time:	2007-127T00:00:01.471	Stop Time:	2007-127T23:59:59.694
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007128_01

Start Time:	2007-128T00:00:06.053	Stop Time:	2007-128T23:59:59.627
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007129_01

Start Time:	2007-129T00:00:03.377	Stop Time:	2007-129T23:59:57.330
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007130_01

Start Time:	2007-130T00:00:01.080	Stop Time:	2007-130T23:59:57.783
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007131_01

Start Time:	2007-131T00:00:01.533	Stop Time:	2007-131T23:59:57.189
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007132_01

Start Time:	2007-132T00:00:03.536	Stop Time:	2007-132T23:59:56.689
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007133_01

Start Time:	2007-133T00:00:02.313	Stop Time:	2007-133T23:59:57.141
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007134_01

Start Time:	2007-134T00:00:00.891	Stop Time:	2007-134T23:59:58.594
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007135_01

Start Time:	2007-135T00:00:02.344	Stop Time:	2007-135T23:59:57.297
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007136_01

Start Time:	2007-136T00:00:01.047	Stop Time:	2007-136T23:59:58.750
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007137_01

Start Time:	2007-137T00:00:02.500	Stop Time:	2007-137T23:59:56.453
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007138_01

Start Time:	2007-138T00:00:00.203	Stop Time:	2007-138T23:59:57.156
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007139_01

Start Time:	2007-139T00:00:01.843	Stop Time:	2007-139T23:59:55.921
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007140_01

Start Time:	2007-140T00:00:00.609	Stop Time:	2007-140T23:59:58.062
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007141_01

Start Time:	2007-141T00:00:01.812	Stop Time:	2007-141T23:59:56.765
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007142_01

Start Time:	2007-142T00:00:00.515	Stop Time:	2007-142T23:59:59.967
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007143_01

Start Time:	2007-143T00:00:04.655	Stop Time:	2007-143T23:59:58.170
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007144_01

Start Time:	2007-144T00:00:01.920	Stop Time:	2007-144T23:59:59.623
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007145_01

Start Time:	2007-145T00:00:03.373	Stop Time:	2007-145T23:59:57.326
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007146_01

Start Time:	2007-146T00:00:01.076	Stop Time:	2007-146T23:59:59.654
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007147_01

Start Time:	2007-147T00:00:04.341	Stop Time:	2007-147T23:59:53.712
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007148_01

Start Time:	2007-148T00:00:00.037	Stop Time:	2007-148T23:59:58.685
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007149_01

Start Time:	2007-149T00:00:04.310	Stop Time:	2007-149T23:59:59.138
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007150_01

Start Time:	2007-150T00:00:02.888	Stop Time:	2007-150T23:59:57.391
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007151_01

Start Time:	2007-151T00:00:03.759	Stop Time:	2007-151T23:59:50.317
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007152_01

Start Time:	2007-152T00:00:01.547	Stop Time:	2007-152T23:59:58.996
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007153_01

Start Time:	2007-153T00:00:02.746	Stop Time:	2007-153T23:59:59.199
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007154_01

Start Time:	2007-154T00:00:02.949	Stop Time:	2007-154T23:59:57.301
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007155_01

Start Time:	2007-155T00:00:03.906	Stop Time:	2007-155T23:59:55.898
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007156_01

Start Time:	2007-156T00:00:02.214	Stop Time:	2007-156T23:59:56.808
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007157_01

Start Time:	2007-157T00:00:00.558	Stop Time:	2007-157T23:59:58.261
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007158_01

Start Time:	2007-158T00:00:02.011	Stop Time:	2007-158T23:59:58.729
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007159_01

Start Time:	2007-159T00:00:05.030	Stop Time:	2007-159T21:36:11.143
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007160_01

Start Time:	2007-160T02:54:50.104	Stop Time:	2007-160T23:59:57.119
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007161_01

Start Time:	2007-161T00:00:00.869	Stop Time:	2007-161T23:59:59.510
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007162_01

Start Time:	2007-162T00:00:04.197	Stop Time:	2007-162T23:59:56.275
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007163_01

Start Time:	2007-163T00:00:00.025	Stop Time:	2007-163T23:59:57.982
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007164_01

Start Time:	2007-164T00:00:00.791	Stop Time:	2007-164T23:59:59.431
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007165_01

Start Time:	2007-165T00:00:03.181	Stop Time:	2007-165T23:59:59.446
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007166_01

Start Time:	2007-166T00:00:02.259	Stop Time:	2007-166T23:59:59.087
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007167_01

Start Time:	2007-167T00:00:01.899	Stop Time:	2007-167T23:59:58.727
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007168_01

Start Time:	2007-168T00:00:01.540	Stop Time:	2007-168T23:59:58.806
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007169_01

Start Time:	2007-169T00:00:01.619	Stop Time:	2007-169T23:59:57.634
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007170_01

Start Time:	2007-170T00:00:00.446	Stop Time:	2007-170T23:59:57.274
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007171_01

Start Time:	2007-171T00:00:00.087	Stop Time:	2007-171T23:59:54.458
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007172_01

Start Time:	2007-172T00:00:00.743	Stop Time:	2007-172T23:59:57.680
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007173_01

Start Time:	2007-173T00:00:00.493	Stop Time:	2007-173T23:59:57.320
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007174_01

Start Time:	2007-174T00:00:00.133	Stop Time:	2007-174T23:59:57.457
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007175_01

Start Time:	2007-175T00:00:03.734	Stop Time:	2007-175T23:59:58.351
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007176_01

Start Time:	2007-176T00:00:01.164	Stop Time:	2007-176T23:59:59.117
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007177_01

Start Time:	2007-177T00:00:05.492	Stop Time:	2007-177T23:59:56.882
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007178_01

Start Time:	2007-178T00:00:01.569	Stop Time:	2007-178T23:59:59.522
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007179_01

Start Time:	2007-179T00:00:03.272	Stop Time:	2007-179T23:59:56.475
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007180_01

Start Time:	2007-180T00:00:02.100	Stop Time:	2007-180T23:59:56.928
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007181_01

Start Time:	2007-181T00:00:00.678	Stop Time:	2007-181T23:59:57.381
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007182_01

Start Time:	2007-182T00:00:00.194	Stop Time:	2007-182T23:59:58.850
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007183_01

Start Time:	2007-183T00:00:05.103	Stop Time:	2007-183T23:59:57.728
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007184_01

Start Time:	2007-184T00:00:03.998	Stop Time:	2007-184T23:59:59.990
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007185_01

Start Time:	2007-185T00:00:03.740	Stop Time:	2007-185T23:59:56.443
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007186_01

Start Time:	2007-186T00:00:00.193	Stop Time:	2007-186T23:59:56.474
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007187_01

Start Time:	2007-187T00:00:02.743	Stop Time:	2007-187T23:59:57.512
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007188_01

Start Time:	2007-188T00:00:03.790	Stop Time:	2007-188T23:59:54.747
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007189_01

Start Time:	2007-189T00:00:01.063	Stop Time:	2007-189T23:59:59.629
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007190_01

Start Time:	2007-190T00:00:02.442	Stop Time:	2007-190T23:59:57.457
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007191_01

Start Time:	2007-191T00:00:00.269	Stop Time:	2007-191T23:59:55.797
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007192_01

Start Time:	2007-192T00:00:02.082	Stop Time:	2007-192T23:59:58.449
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007193_01

Start Time:	2007-193T00:00:04.785	Stop Time:	2007-193T23:59:57.394
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007194_01

Start Time:	2007-194T00:00:03.655	Stop Time:	2007-194T23:59:57.456
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007195_01

Start Time:	2007-195T00:00:00.269	Stop Time:	2007-195T23:59:58.475
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007196_01

Start Time:	2007-196T00:00:01.284	Stop Time:	2007-196T23:59:59.112
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007197_01

Start Time:	2007-197T00:00:01.928	Stop Time:	2007-197T23:59:58.752
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007198_01

Start Time:	2007-198T00:00:01.565	Stop Time:	2007-198T23:59:57.299
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007199_01

Start Time:	2007-199T00:00:03.592	Stop Time:	2007-199T23:59:59.658
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007200_01

Start Time:	2007-200T00:00:02.470	Stop Time:	2007-200T23:59:59.298
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007201_01

Start Time:	2007-201T00:00:02.111	Stop Time:	2007-201T23:59:57.439
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007202_01

Start Time:	2007-202T00:00:01.189	Stop Time:	2007-202T23:59:58.892
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007203_01

Start Time:	2007-203T00:00:03.579	Stop Time:	2007-203T23:59:54.954
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007204_01

Start Time:	2007-204T00:00:01.270	Stop Time:	2007-204T23:59:56.048
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007205_01

Start Time:	2007-205T00:00:00.736	Stop Time:	2007-205T23:59:59.376
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007206_01

Start Time:	2007-206T00:00:04.064	Stop Time:	2007-206T23:59:58.704
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007207_01

Start Time:	2007-207T00:00:02.454	Stop Time:	2007-207T23:59:54.614
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007208_01

Start Time:	2007-208T00:00:00.899	Stop Time:	2007-208T23:59:59.762
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007209_01

Start Time:	2007-209T00:00:10.946	Stop Time:	2007-209T23:59:56.817
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007210_01

Start Time:	2007-210T00:00:00.563	Stop Time:	2007-210T23:59:58.270
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007211_01

Start Time:	2007-211T00:00:02.016	Stop Time:	2007-211T23:59:51.305
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007212_01

Start Time:	2007-212T00:00:02.492	Stop Time:	2007-212T23:59:57.422
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007213_01

Start Time:	2007-213T00:00:01.171	Stop Time:	2007-213T23:59:57.874
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007214_01

Start Time:	2007-214T00:00:01.624	Stop Time:	2007-214T23:59:57.577
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007215_01

Start Time:	2007-215T00:00:01.327	Stop Time:	2007-215T23:59:56.933
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007216_01

Start Time:	2007-216T00:00:08.116	Stop Time:	2007-216T23:59:58.233
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007217_01

Start Time:	2007-217T00:00:01.983	Stop Time:	2007-217T23:59:56.936
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007218_01

Start Time:	2007-218T00:00:00.686	Stop Time:	2007-218T23:59:57.139
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007219_01

Start Time:	2007-219T00:00:00.889	Stop Time:	2007-219T23:59:58.842
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007220_01

Start Time:	2007-220T00:00:02.592	Stop Time:	2007-220T23:59:56.295
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007221_01

Start Time:	2007-221T00:00:00.045	Stop Time:	2007-221T23:59:56.747
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007222_01

Start Time:	2007-222T00:00:00.497	Stop Time:	2007-222T23:59:58.200
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007223_01

Start Time:	2007-223T00:00:01.950	Stop Time:	2007-223T23:59:59.653
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007224_01

Start Time:	2007-224T00:00:05.278	Stop Time:	2007-224T23:59:54.610
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007225_01

Start Time:	2007-225T00:00:00.231	Stop Time:	2007-225T23:59:55.063
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007226_01

Start Time:	2007-226T00:00:00.684	Stop Time:	2007-226T23:59:55.637
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007227_01

Start Time:	2007-227T00:00:01.262	Stop Time:	2007-227T23:59:57.465
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007228_01

Start Time:	2007-228T00:00:03.090	Stop Time:	2007-228T23:59:56.293
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007229_01

Start Time:	2007-229T00:00:01.918	Stop Time:	2007-229T23:59:56.371
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007230_01

Start Time:	2007-230T00:00:01.996	Stop Time:	2007-230T23:59:58.929
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007231_01

Start Time:	2007-231T00:00:05.230	Stop Time:	2007-231T23:59:59.026
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007232_01

Start Time:	2007-232T00:00:02.780	Stop Time:	2007-232T23:59:56.729
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007233_01

Start Time:	2007-233T00:00:00.479	Stop Time:	2007-233T23:59:58.182
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007234_01

Start Time:	2007-234T00:00:01.932	Stop Time:	2007-234T23:59:59.635
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007235_01

Start Time:	2007-235T00:00:03.385	Stop Time:	2007-235T23:59:57.338
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007236_01

Start Time:	2007-236T00:00:01.088	Stop Time:	2007-236T23:59:56.045
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007237_01

Start Time:	2007-237T00:00:02.408	Stop Time:	2007-237T23:59:58.744
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007238_01

Start Time:	2007-238T00:00:04.369	Stop Time:	2007-238T23:59:54.697
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007239_01

Start Time:	2007-239T00:00:00.322	Stop Time:	2007-239T23:59:58.900
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007240_01

Start Time:	2007-240T00:00:02.650	Stop Time:	2007-240T23:59:56.602
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007241_01

Start Time:	2007-241T00:00:00.352	Stop Time:	2007-241T23:59:58.055
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007242_01

Start Time:	2007-242T00:00:01.805	Stop Time:	2007-242T23:59:56.008
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007243_01

Start Time:	2007-243T00:00:01.633	Stop Time:	2007-243T23:59:57.461
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007244_01

Start Time:	2007-244T00:00:01.211	Stop Time:	2007-244T23:59:59.789
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007245_01

Start Time:	2007-245T00:00:05.414	Stop Time:	2007-245T23:59:58.992
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007246_01

Start Time:	2007-246T00:00:04.617	Stop Time:	2007-246T23:59:54.945
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007247_01

Start Time:	2007-247T00:00:00.574	Stop Time:	2007-247T23:59:54.398
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007248_01

Start Time:	2007-248T00:00:00.027	Stop Time:	2007-248T23:59:59.351
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007249_01

Start Time:	2007-249T00:00:04.976	Stop Time:	2007-249T23:59:55.429
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007250_01

Start Time:	2007-250T00:00:01.054	Stop Time:	2007-250T23:59:56.006
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007251_01

Start Time:	2007-251T00:00:01.631	Stop Time:	2007-251T23:59:56.084
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007252_01

Start Time:	2007-252T00:00:01.709	Stop Time:	2007-252T23:59:54.787
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007253_01

Start Time:	2007-253T00:00:00.412	Stop Time:	2007-253T23:59:58.616
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007254_01

Start Time:	2007-254T00:00:04.241	Stop Time:	2007-254T06:17:34.973
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007258_01

Start Time:	2007-258T18:08:35.143	Stop Time:	2007-258T21:41:55.558
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007259_01

Start Time:	2007-259T12:06:02.734	Stop Time:	2007-259T23:59:58.459
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007260_01

Start Time:	2007-260T00:00:05.958	Stop Time:	2007-260T23:59:54.911
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007261_01

Start Time:	2007-261T00:00:02.411	Stop Time:	2007-261T23:59:55.864
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007262_01

Start Time:	2007-262T00:00:03.364	Stop Time:	2007-262T23:59:59.817
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007263_01

Start Time:	2007-263T00:00:07.317	Stop Time:	2007-263T23:59:55.770
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007264_01

Start Time:	2007-264T00:00:03.274	Stop Time:	2007-264T23:59:55.223
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007265_01

Start Time:	2007-265T00:00:02.723	Stop Time:	2007-265T23:59:56.676
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007266_01

Start Time:	2007-266T00:00:02.301	Stop Time:	2007-266T23:59:55.129
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007267_01

Start Time:	2007-267T00:00:00.754	Stop Time:	2007-267T23:59:56.394
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007268_01

Start Time:	2007-268T00:00:01.086	Stop Time:	2007-268T23:59:58.535
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007269_01

Start Time:	2007-269T00:00:02.285	Stop Time:	2007-269T20:54:24.293
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007270_01

Start Time:	2007-270T14:25:38.648	Stop Time:	2007-270T23:59:56.426
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007271_01

Start Time:	2007-271T00:00:00.176	Stop Time:	2007-271T23:59:57.880
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007272_01

Start Time:	2007-272T00:00:01.630	Stop Time:	2007-272T23:59:59.333
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007273_01

Start Time:	2007-273T00:00:03.083	Stop Time:	2007-273T22:11:45.077
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007274_01

Start Time:	2007-274T12:30:50.204	Stop Time:	2007-274T23:59:58.739
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007275_01

Start Time:	2007-275T00:00:02.489	Stop Time:	2007-275T08:02:45.431
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007276_01

Start Time:	2007-276T13:38:44.893	Stop Time:	2007-276T23:59:56.271
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007277_01

Start Time:	2007-277T00:00:01.896	Stop Time:	2007-277T23:59:58.474
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007278_01

Start Time:	2007-278T00:00:04.099	Stop Time:	2007-278T23:59:57.552
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007279_01

Start Time:	2007-279T00:00:03.177	Stop Time:	2007-279T20:20:40.964
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007291_01

Start Time:	2007-291T19:32:47.357	Stop Time:	2007-291T23:59:57.489
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007292_01

Start Time:	2007-292T00:00:03.114	Stop Time:	2007-292T23:59:59.122
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007293_01

Start Time:	2007-293T00:00:04.747	Stop Time:	2007-293T23:59:58.381
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007294_01

Start Time:	2007-294T00:00:04.006	Stop Time:	2007-294T23:59:59.265
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007295_01

Start Time:	2007-295T00:00:04.890	Stop Time:	2007-295T23:59:58.273
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007296_01

Start Time:	2007-296T00:00:02.023	Stop Time:	2007-296T23:59:59.657
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007297_01

Start Time:	2007-297T00:00:03.407	Stop Time:	2007-297T23:59:57.324
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007298_01

Start Time:	2007-298T00:00:01.074	Stop Time:	2007-298T23:59:58.716
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007299_01

Start Time:	2007-299T00:00:02.466	Stop Time:	2007-299T23:59:56.358
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007300_01

Start Time:	2007-300T00:00:00.108	Stop Time:	2007-300T23:59:56.251
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007301_01

Start Time:	2007-301T00:00:00.001	Stop Time:	2007-301T23:59:57.143
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007302_01

Start Time:	2007-302T00:00:00.893	Stop Time:	2007-302T23:59:55.660
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007303_01

Start Time:	2007-303T00:00:00.348	Stop Time:	2007-303T23:59:57.932
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007304_01

Start Time:	2007-304T00:00:01.678	Stop Time:	2007-304T23:59:59.382
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007305_01

Start Time:	2007-305T00:00:02.194	Stop Time:	2007-305T23:59:58.462
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007306_01

Start Time:	2007-306T00:00:01.274	Stop Time:	2007-306T23:59:57.604
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007307_01

Start Time:	2007-307T00:00:00.416	Stop Time:	2007-307T23:59:56.996
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007308_01

Start Time:	2007-308T00:00:00.746	Stop Time:	2007-308T23:59:58.389
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007309_01

Start Time:	2007-309T00:00:02.139	Stop Time:	2007-309T23:59:57.781
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007310_01

Start Time:	2007-310T00:00:01.531	Stop Time:	2007-310T23:59:58.877
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007311_01

Start Time:	2007-311T00:00:02.627	Stop Time:	2007-311T23:59:58.267
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007312_01

Start Time:	2007-312T00:00:02.017	Stop Time:	2007-312T23:59:58.156
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007313_01

Start Time:	2007-313T00:00:01.906	Stop Time:	2007-313T23:59:57.671
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007314_01

Start Time:	2007-314T00:00:00.483	Stop Time:	2007-314T23:59:58.310
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007315_01

Start Time:	2007-315T00:00:03.935	Stop Time:	2007-315T23:59:54.575
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007316_01

Start Time:	2007-316T00:00:00.200	Stop Time:	2007-316T23:59:59.340
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007317_01

Start Time:	2007-317T00:00:04.965	Stop Time:	2007-317T23:59:57.358
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007318_01

Start Time:	2007-318T00:00:02.979	Stop Time:	2007-318T23:59:58.619
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007319_01

Start Time:	2007-319T00:00:04.244	Stop Time:	2007-319T23:59:59.633
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007320_01

Start Time:	2007-320T00:00:03.383	Stop Time:	2007-320T23:59:58.023
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007321_01

Start Time:	2007-321T00:00:01.773	Stop Time:	2007-321T23:59:59.413
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007322_01

Start Time:	2007-322T00:00:03.163	Stop Time:	2007-322T23:59:58.052
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007323_01

Start Time:	2007-323T00:00:00.865	Stop Time:	2007-323T23:59:59.442
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007324_01

Start Time:	2007-324T00:00:03.192	Stop Time:	2007-324T23:59:58.331
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007325_01

Start Time:	2007-325T00:00:01.144	Stop Time:	2007-325T23:59:57.908
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007326_01

Start Time:	2007-326T00:00:00.721	Stop Time:	2007-326T23:59:58.423
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007327_01

Start Time:	2007-327T00:00:01.236	Stop Time:	2007-327T23:59:58.438
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007328_01

Start Time:	2007-328T00:00:01.254	Stop Time:	2007-328T23:59:57.327
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007329_01

Start Time:	2007-329T00:00:00.140	Stop Time:	2007-329T23:59:59.154
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007330_01

Start Time:	2007-330T00:00:01.967	Stop Time:	2007-330T23:59:58.856
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007331_01

Start Time:	2007-331T00:00:01.669	Stop Time:	2007-331T23:59:58.996
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007332_01

Start Time:	2007-332T00:00:01.812	Stop Time:	2007-332T23:59:58.948
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007333_01

Start Time:	2007-333T00:00:02.698	Stop Time:	2007-333T23:59:58.463
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007334_01

Start Time:	2007-334T00:00:03.150	Stop Time:	2007-334T23:59:57.977
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007335_01

Start Time:	2007-335T00:00:01.727	Stop Time:	2007-335T23:59:59.367
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007336_01

Start Time:	2007-336T00:00:03.117	Stop Time:	2007-336T23:59:59.819
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007337_01

Start Time:	2007-337T00:00:02.632	Stop Time:	2007-337T23:59:57.146
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007338_01

Start Time:	2007-338T00:00:00.896	Stop Time:	2007-338T23:59:59.473
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007339_01

Start Time:	2007-339T00:00:02.286	Stop Time:	2007-339T23:59:57.050
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007340_01

Start Time:	2007-340T00:00:02.675	Stop Time:	2007-340T23:59:57.440
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007341_01

Start Time:	2007-341T00:00:03.065	Stop Time:	2007-341T23:59:59.830
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007342_01

Start Time:	2007-342T00:00:02.642	Stop Time:	2007-342T23:59:57.594
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007343_01

Start Time:	2007-343T00:00:00.407	Stop Time:	2007-343T23:59:59.921
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007344_01

Start Time:	2007-344T00:00:02.734	Stop Time:	2007-344T23:59:58.186
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007345_01

Start Time:	2007-345T00:00:00.998	Stop Time:	2007-345T23:59:59.513
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007346_01

Start Time:	2007-346T00:00:02.326	Stop Time:	2007-346T17:41:47.000
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007347_01

Start Time:	2007-347T01:05:52.629	Stop Time:	2007-347T09:44:58.592
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007348_01

Start Time:	2007-348T15:54:33.642	Stop Time:	2007-348T23:59:58.682
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007349_01

Start Time:	2007-349T00:00:04.307	Stop Time:	2007-349T23:59:59.071
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007350_01

Start Time:	2007-350T00:00:04.696	Stop Time:	2007-350T23:59:59.461
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007351_01

Start Time:	2007-351T00:00:05.086	Stop Time:	2007-351T23:59:58.037
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007352_01

Start Time:	2007-352T00:00:00.850	Stop Time:	2007-352T23:59:58.648
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007353_01

Start Time:	2007-353T00:00:01.461	Stop Time:	2007-353T23:59:59.725
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007354_01

Start Time:	2007-354T00:00:02.538	Stop Time:	2007-354T23:59:59.303
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007355_01

Start Time:	2007-355T00:00:02.115	Stop Time:	2007-355T23:59:59.692
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007356_01

Start Time:	2007-356T00:00:02.505	Stop Time:	2007-356T23:59:59.332
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007357_01

Start Time:	2007-357T00:00:03.082	Stop Time:	2007-357T23:59:56.971
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007358_01

Start Time:	2007-358T00:00:00.721	Stop Time:	2007-358T23:59:58.361
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007359_01

Start Time:	2007-359T00:00:02.111	Stop Time:	2007-359T23:59:58.876
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007360_01

Start Time:	2007-360T00:00:01.688	Stop Time:	2007-360T23:59:59.144
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007361_01

Start Time:	2007-361T00:00:05.476	Stop Time:	2007-361T23:59:58.655
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007362_01

Start Time:	2007-362T00:00:01.467	Stop Time:	2007-362T23:59:58.169
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007363_01

Start Time:	2007-363T00:00:01.919	Stop Time:	2007-363T23:59:58.559
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007364_01

Start Time:	2007-364T00:00:02.313	Stop Time:	2007-364T23:59:58.199
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2007365_01

Start Time:	2007-365T00:00:01.949	Stop Time:	2007-365T23:59:59.088
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

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