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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/ 2015 /

LACCFULL0_2015001_01

Start Time:	2015-001T00:00:02.317	Stop Time:	2015-001T23:59:58.048
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_2015002_01

Start Time:	2015-002T00:00:03.673	Stop Time:	2015-002T23:59:55.377
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015003_01

Start Time:	2015-003T00:00:00.998	Stop Time:	2015-003T23:59:55.826
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015004_01

Start Time:	2015-004T00:00:01.447	Stop Time:	2015-004T23:59:58.647
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015005_01

Start Time:	2015-005T00:00:04.275	Stop Time:	2015-005T23:59:59.346
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015006_01

Start Time:	2015-006T00:00:04.971	Stop Time:	2015-006T23:59:53.096
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015007_01

Start Time:	2015-007T00:00:01.092	Stop Time:	2015-007T23:59:57.745
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015008_01

Start Time:	2015-008T00:00:05.768	Stop Time:	2015-008T23:59:56.195
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015009_01

Start Time:	2015-009T00:00:01.819	Stop Time:	2015-009T23:59:55.644
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015010_01

Start Time:	2015-010T00:00:01.269	Stop Time:	2015-010T23:59:59.843
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015011_01

Start Time:	2015-011T00:00:05.468	Stop Time:	2015-011T23:59:56.543
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015012_01

Start Time:	2015-012T00:00:02.168	Stop Time:	2015-012T23:59:56.117
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_2015013_01

Start Time:	2015-013T00:00:01.742	Stop Time:	2015-013T23:59:56.567
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015014_01

Start Time:	2015-014T00:00:02.192	Stop Time:	2015-014T23:59:58.891
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015015_01

Start Time:	2015-015T00:00:04.516	Stop Time:	2015-015T23:59:54.716
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_2015016_01

Start Time:	2015-016T00:00:00.341	Stop Time:	2015-016T23:59:59.915
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_2015017_01

Start Time:	2015-017T00:00:03.669	Stop Time:	2015-017T23:59:54.740
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015018_01

Start Time:	2015-018T00:00:00.365	Stop Time:	2015-018T23:59:59.814
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015019_01

Start Time:	2015-019T00:00:05.439	Stop Time:	2015-019T23:59:54.639
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015020_01

Start Time:	2015-020T00:00:00.264	Stop Time:	2015-020T23:59:55.088
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.

LACCFULL0_2015021_01

Start Time:	2015-021T00:00:00.713	Stop Time:	2015-021T23:59:59.287
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015022_01

Start Time:	2015-022T00:00:04.916	Stop Time:	2015-022T23:59:59.736
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015023_01

Start Time:	2015-023T00:00:05.365	Stop Time:	2015-023T23:59:58.686
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015024_01

Start Time:	2015-024T00:00:04.311	Stop Time:	2015-024T23:59:55.010
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015025_01

Start Time:	2015-025T00:00:00.635	Stop Time:	2015-025T23:59:56.460
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015026_01

Start Time:	2015-026T00:00:02.085	Stop Time:	2015-026T23:59:56.909
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015027_01

Start Time:	2015-027T00:00:02.534	Stop Time:	2015-027T23:59:56.913
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_2015028_01

Start Time:	2015-028T00:00:06.577	Stop Time:	2015-028T23:59:54.808
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_2015029_01

Start Time:	2015-029T00:00:00.433	Stop Time:	2015-029T23:59:55.008
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_2015030_01

Start Time:	2015-030T00:00:00.633	Stop Time:	2015-030T23:59:55.457
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_2015031_01

Start Time:	2015-031T00:00:01.082	Stop Time:	2015-031T23:59:55.657
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_2015032_01

Start Time:	2015-032T00:00:01.281	Stop Time:	2015-032T23:59:55.481
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015033_01

Start Time:	2015-033T00:00:01.106	Stop Time:	2015-033T23:59:54.930
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015034_01

Start Time:	2015-034T00:00:00.555	Stop Time:	2015-034T23:59:56.880
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_2015035_01

Start Time:	2015-035T00:00:02.505	Stop Time:	2015-035T23:59:57.329
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015036_01

Start Time:	2015-036T00:00:02.954	Stop Time:	2015-036T23:59:54.904
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015037_01

Start Time:	2015-037T00:00:00.529	Stop Time:	2015-037T23:59:54.978
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015038_01

Start Time:	2015-038T00:00:00.603	Stop Time:	2015-038T23:59:55.428
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015039_01

Start Time:	2015-039T00:00:01.053	Stop Time:	2015-039T23:59:55.877
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_2015040_01

Start Time:	2015-040T00:00:01.502	Stop Time:	2015-040T23:59:58.077
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_2015041_01

Start Time:	2015-041T00:00:03.702	Stop Time:	2015-041T23:59:54.776
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015042_01

Start Time:	2015-042T00:00:00.401	Stop Time:	2015-042T23:59:57.976
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015043_01

Start Time:	2015-043T00:00:03.601	Stop Time:	2015-043T23:59:56.550
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015044_01

Start Time:	2015-044T00:00:00.300	Stop Time:	2015-044T23:59:56.336
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015045_01

Start Time:	2015-045T00:00:04.355	Stop Time:	2015-045T23:59:56.449
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_2015046_01

Start Time:	2015-046T00:00:00.199	Stop Time:	2015-046T23:59:57.649
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015047_01

Start Time:	2015-047T00:00:01.399	Stop Time:	2015-047T23:59:56.598
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015048_01

Start Time:	2015-048T00:00:02.223	Stop Time:	2015-048T23:59:55.798
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015049_01

Start Time:	2015-049T00:00:01.423	Stop Time:	2015-049T23:59:59.997
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015050_01

Start Time:	2015-050T00:00:03.747	Stop Time:	2015-050T23:59:59.696
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015051_01

Start Time:	2015-051T00:00:03.446	Stop Time:	2015-051T23:59:54.646
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015052_01

Start Time:	2015-052T00:00:00.271	Stop Time:	2015-052T23:59:55.095
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015053_01

Start Time:	2015-053T00:00:00.720	Stop Time:	2015-053T23:59:54.545
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015054_01

Start Time:	2015-054T00:00:00.170	Stop Time:	2015-054T23:59:58.369
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_2015055_01

Start Time:	2015-055T00:00:03.994	Stop Time:	2015-055T23:59:57.819
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_2015056_01

Start Time:	2015-056T00:00:03.444	Stop Time:	2015-056T23:59:56.643
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015057_01

Start Time:	2015-057T00:00:00.393	Stop Time:	2015-057T23:59:56.218
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015058_01

Start Time:	2015-058T00:00:01.843	Stop Time:	2015-058T23:59:58.667
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015059_01

Start Time:	2015-059T00:00:04.292	Stop Time:	2015-059T23:59:57.242
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015060_01

Start Time:	2015-060T00:00:02.867	Stop Time:	2015-060T23:59:58.316
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015061_01

Start Time:	2015-061T00:00:03.941	Stop Time:	2015-061T23:59:58.516
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015062_01

Start Time:	2015-062T00:00:04.141	Stop Time:	2015-062T23:59:56.090
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015063_01

Start Time:	2015-063T00:00:01.715	Stop Time:	2015-063T23:59:57.290
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015064_01

Start Time:	2015-064T00:00:02.915	Stop Time:	2015-064T23:59:56.239
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015065_01

Start Time:	2015-065T00:00:01.864	Stop Time:	2015-065T23:59:56.688
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015066_01

Start Time:	2015-066T00:00:02.313	Stop Time:	2015-066T23:59:57.638
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015067_01

Start Time:	2015-067T00:00:03.263	Stop Time:	2015-067T23:59:58.087
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_2015068_01

Start Time:	2015-068T00:00:03.712	Stop Time:	2015-068T23:59:55.286
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015069_01

Start Time:	2015-069T00:00:00.911	Stop Time:	2015-069T23:59:59.110
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015070_01

Start Time:	2015-070T00:00:04.735	Stop Time:	2015-070T23:59:59.560
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015071_01

Start Time:	2015-071T00:00:05.185	Stop Time:	2015-071T23:59:59.009
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015072_01

Start Time:	2015-072T00:00:04.634	Stop Time:	2015-072T23:59:58.959
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015073_01

Start Time:	2015-073T00:00:04.584	Stop Time:	2015-073T23:59:59.283
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015074_01

Start Time:	2015-074T00:00:04.908	Stop Time:	2015-074T23:59:59.733
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015075_01

Start Time:	2015-075T00:00:05.358	Stop Time:	2015-075T23:59:57.432
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015076_01

Start Time:	2015-076T00:00:01.186	Stop Time:	2015-076T23:59:58.507
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015077_01

Start Time:	2015-077T00:00:04.132	Stop Time:	2015-077T23:59:59.831
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015078_01

Start Time:	2015-078T00:00:03.581	Stop Time:	2015-078T23:59:56.780
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015079_01

Start Time:	2015-079T00:00:02.405	Stop Time:	2015-079T23:59:59.730
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_2015080_01

Start Time:	2015-080T00:00:03.480	Stop Time:	2015-080T23:59:57.429
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_2015081_01

Start Time:	2015-081T00:00:01.179	Stop Time:	2015-081T23:59:58.129
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_2015082_01

Start Time:	2015-082T00:00:01.879	Stop Time:	2015-082T23:59:54.828
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015083_01

Start Time:	2015-083T00:00:00.453	Stop Time:	2015-083T23:59:58.778
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015084_01

Start Time:	2015-084T00:00:02.528	Stop Time:	2015-084T23:59:58.352
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015085_01

Start Time:	2015-085T00:00:03.977	Stop Time:	2015-085T23:59:57.052
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_2015086_01

Start Time:	2015-086T00:00:02.681	Stop Time:	2015-086T23:59:57.501
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015087_01

Start Time:	2015-087T00:00:03.130	Stop Time:	2015-087T23:59:54.861
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015088_01

Start Time:	2015-088T00:00:02.908	Stop Time:	2015-088T23:59:58.150
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015089_01

Start Time:	2015-089T00:00:03.775	Stop Time:	2015-089T23:59:57.599
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015090_01

Start Time:	2015-090T00:00:03.224	Stop Time:	2015-090T23:59:59.049
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015091_01

Start Time:	2015-091T00:00:04.674	Stop Time:	2015-091T23:59:59.955
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015092_01

Start Time:	2015-092T00:00:07.885	Stop Time:	2015-092T23:59:56.948
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_2015093_01

Start Time:	2015-093T00:00:02.573	Stop Time:	2015-093T23:59:53.229
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015094_01

Start Time:	2015-094T00:00:01.315	Stop Time:	2015-094T23:59:57.726
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015095_01

Start Time:	2015-095T00:00:03.347	Stop Time:	2015-095T23:59:52.163
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015096_01

Start Time:	2015-096T00:00:00.156	Stop Time:	2015-096T23:59:58.746
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015097_01

Start Time:	2015-097T00:00:04.371	Stop Time:	2015-097T23:59:58.445
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015098_01

Start Time:	2015-098T00:00:04.074	Stop Time:	2015-098T23:59:58.895
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_2015099_01

Start Time:	2015-099T00:00:04.523	Stop Time:	2015-099T23:59:57.844
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015100_01

Start Time:	2015-100T00:00:03.469	Stop Time:	2015-100T23:59:59.231
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015101_01

Start Time:	2015-101T00:00:07.200	Stop Time:	2015-101T23:59:58.305
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_2015102_01

Start Time:	2015-102T00:00:04.872	Stop Time:	2015-102T23:59:58.817
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_2015103_01

Start Time:	2015-103T00:00:02.567	Stop Time:	2015-103T23:59:56.517
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015104_01

Start Time:	2015-104T00:00:00.267	Stop Time:	2015-104T23:59:56.091
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015105_01

Start Time:	2015-105T00:00:01.716	Stop Time:	2015-105T23:59:54.666
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015106_01

Start Time:	2015-106T00:00:00.291	Stop Time:	2015-106T23:59:56.990
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_2015107_01

Start Time:	2015-107T00:00:02.615	Stop Time:	2015-107T23:59:59.315
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015108_01

Start Time:	2015-108T00:00:03.065	Stop Time:	2015-108T23:59:59.764
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015109_01

Start Time:	2015-109T00:00:03.514	Stop Time:	2015-109T23:59:57.463
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_2015110_01

Start Time:	2015-110T00:00:01.213	Stop Time:	2015-110T23:59:56.038
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015111_01

Start Time:	2015-111T00:00:01.663	Stop Time:	2015-111T23:59:56.487
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015112_01

Start Time:	2015-112T00:00:02.112	Stop Time:	2015-112T23:59:55.937
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015113_01

Start Time:	2015-113T00:00:01.562	Stop Time:	2015-113T23:59:56.011
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015114_01

Start Time:	2015-114T00:00:01.636	Stop Time:	2015-114T23:59:56.461
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_2015115_01

Start Time:	2015-115T00:00:02.086	Stop Time:	2015-115T23:59:57.164
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015116_01

Start Time:	2015-116T00:00:00.910	Stop Time:	2015-116T23:59:56.735
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015117_01

Start Time:	2015-117T00:00:02.359	Stop Time:	2015-117T23:59:56.684
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015118_01

Start Time:	2015-118T00:00:02.309	Stop Time:	2015-118T23:59:56.133
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015119_01

Start Time:	2015-119T00:00:01.758	Stop Time:	2015-119T23:59:56.584
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015120_01

Start Time:	2015-120T00:00:02.209	Stop Time:	2015-120T23:59:56.658
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_2015121_01

Start Time:	2015-121T00:00:00.408	Stop Time:	2015-121T23:59:58.983
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015122_01

Start Time:	2015-122T00:00:04.608	Stop Time:	2015-122T23:59:55.311
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015123_01

Start Time:	2015-123T00:00:00.932	Stop Time:	2015-123T23:59:54.882
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_2015124_01

Start Time:	2015-124T00:00:00.507	Stop Time:	2015-124T23:59:56.210
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015125_01

Start Time:	2015-125T00:00:01.831	Stop Time:	2015-125T23:59:56.405
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015126_01

Start Time:	2015-126T00:00:02.030	Stop Time:	2015-126T23:59:55.855
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015127_01

Start Time:	2015-127T00:00:01.480	Stop Time:	2015-127T23:59:57.304
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015128_01

Start Time:	2015-128T00:00:01.054	Stop Time:	2015-128T23:59:56.996
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_2015129_01

Start Time:	2015-129T00:00:04.988	Stop Time:	2015-129T23:59:56.453
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_2015130_01

Start Time:	2015-130T00:00:00.203	Stop Time:	2015-130T23:59:59.653
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_2015131_01

Start Time:	2015-131T00:00:03.403	Stop Time:	2015-131T23:59:58.727
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_2015132_01

Start Time:	2015-132T00:00:04.356	Stop Time:	2015-132T23:59:58.301
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_2015133_01

Start Time:	2015-133T00:00:02.051	Stop Time:	2015-133T23:59:59.751
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015134_01

Start Time:	2015-134T00:00:03.501	Stop Time:	2015-134T23:59:56.450
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_2015135_01

Start Time:	2015-135T00:00:00.200	Stop Time:	2015-135T23:59:58.775
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015136_01

Start Time:	2015-136T00:00:04.400	Stop Time:	2015-136T23:59:59.224
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015137_01

Start Time:	2015-137T00:00:04.849	Stop Time:	2015-137T23:59:58.674
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015138_01

Start Time:	2015-138T00:00:04.299	Stop Time:	2015-138T23:59:59.123
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015139_01

Start Time:	2015-139T00:00:04.748	Stop Time:	2015-139T23:59:59.572
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015140_01

Start Time:	2015-140T00:00:05.197	Stop Time:	2015-140T23:59:57.647
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015141_01

Start Time:	2015-141T00:00:03.272	Stop Time:	2015-141T23:59:57.096
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015142_01

Start Time:	2015-142T00:00:02.721	Stop Time:	2015-142T23:59:54.921
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_2015143_01

Start Time:	2015-143T00:00:00.546	Stop Time:	2015-143T23:59:59.995
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015144_01

Start Time:	2015-144T00:00:05.620	Stop Time:	2015-144T23:59:58.070
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015145_01

Start Time:	2015-145T00:00:03.695	Stop Time:	2015-145T23:59:58.519
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015146_01

Start Time:	2015-146T00:00:04.144	Stop Time:	2015-146T23:59:56.219
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015147_01

Start Time:	2015-147T00:00:01.843	Stop Time:	2015-147T23:59:56.668
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015148_01

Start Time:	2015-148T00:00:02.293	Stop Time:	2015-148T23:59:58.992
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_2015149_01

Start Time:	2015-149T00:00:02.742	Stop Time:	2015-149T23:59:58.942
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015150_01

Start Time:	2015-150T00:00:02.692	Stop Time:	2015-150T23:59:53.333
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_2015151_01

Start Time:	2015-151T00:00:01.407	Stop Time:	2015-151T23:59:56.341
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015152_01

Start Time:	2015-152T00:00:00.091	Stop Time:	2015-152T23:59:56.794
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015153_01

Start Time:	2015-153T00:00:00.540	Stop Time:	2015-153T23:59:56.365
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015154_01

Start Time:	2015-154T00:00:01.989	Stop Time:	2015-154T23:59:56.814
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015155_01

Start Time:	2015-155T00:00:02.439	Stop Time:	2015-155T23:59:59.142
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015156_01

Start Time:	2015-156T00:00:04.763	Stop Time:	2015-156T23:59:58.592
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_2015157_01

Start Time:	2015-157T00:00:04.213	Stop Time:	2015-157T23:59:59.041
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015158_01

Start Time:	2015-158T00:00:04.662	Stop Time:	2015-158T23:59:59.491
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015159_01

Start Time:	2015-159T00:00:05.112	Stop Time:	2015-159T23:59:55.186
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_2015160_01

Start Time:	2015-160T00:00:00.811	Stop Time:	2015-160T23:59:56.510
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_2015161_01

Start Time:	2015-161T00:00:02.135	Stop Time:	2015-161T23:59:56.960
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015162_01

Start Time:	2015-162T00:00:02.585	Stop Time:	2015-162T23:59:55.284
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015163_01

Start Time:	2015-163T00:00:00.909	Stop Time:	2015-163T23:59:59.359
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015164_01

Start Time:	2015-164T00:00:04.984	Stop Time:	2015-164T23:59:54.683
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015165_01

Start Time:	2015-165T00:00:00.308	Stop Time:	2015-165T23:59:59.633
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_2015166_01

Start Time:	2015-166T00:00:05.258	Stop Time:	2015-166T23:59:54.457
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_2015167_01

Start Time:	2015-167T00:00:00.082	Stop Time:	2015-167T23:59:57.781
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_2015168_01

Start Time:	2015-168T00:00:01.531	Stop Time:	2015-168T23:59:55.357
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015169_01

Start Time:	2015-169T00:00:00.982	Stop Time:	2015-169T23:59:58.181
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_2015170_01

Start Time:	2015-170T00:00:01.931	Stop Time:	2015-170T23:59:58.631
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_2015171_01

Start Time:	2015-171T00:00:02.381	Stop Time:	2015-171T23:59:56.830
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_2015172_01

Start Time:	2015-172T00:00:00.580	Stop Time:	2015-172T23:59:59.030
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015173_01

Start Time:	2015-173T00:00:02.780	Stop Time:	2015-173T23:59:54.854
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015174_01

Start Time:	2015-174T00:00:00.479	Stop Time:	2015-174T23:59:57.303
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_2015175_01

Start Time:	2015-175T00:00:02.928	Stop Time:	2015-175T23:59:58.628
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015176_01

Start Time:	2015-176T00:00:04.253	Stop Time:	2015-176T23:59:54.452
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015177_01

Start Time:	2015-177T00:00:00.077	Stop Time:	2015-177T23:59:59.277
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015178_01

Start Time:	2015-178T00:00:04.902	Stop Time:	2015-178T23:59:57.226
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015179_01

Start Time:	2015-179T00:00:02.851	Stop Time:	2015-179T23:59:59.801
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_2015180_01

Start Time:	2015-180T00:00:05.425	Stop Time:	2015-180T23:59:55.375
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015181_01

Start Time:	2015-181T00:00:01.000	Stop Time:	2015-181T23:59:55.809
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015182_01

Start Time:	2015-182T00:00:02.789	Stop Time:	2015-182T23:59:54.524
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_2015183_01

Start Time:	2015-183T00:00:00.149	Stop Time:	2015-183T23:59:59.223
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_2015184_01

Start Time:	2015-184T00:00:04.848	Stop Time:	2015-184T23:59:55.891
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015185_01

Start Time:	2015-185T00:00:03.860	Stop Time:	2015-185T23:59:53.653
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_2015186_01

Start Time:	2015-186T00:00:01.661	Stop Time:	2015-186T23:59:56.978
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015187_01

Start Time:	2015-187T00:00:04.947	Stop Time:	2015-187T23:59:56.896
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015188_01

Start Time:	2015-188T00:00:02.521	Stop Time:	2015-188T23:59:59.220
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015189_01

Start Time:	2015-189T00:00:02.970	Stop Time:	2015-189T23:59:59.920
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015190_01

Start Time:	2015-190T00:00:03.670	Stop Time:	2015-190T23:59:56.244
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015191_01

Start Time:	2015-191T00:00:01.869	Stop Time:	2015-191T23:59:56.694
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_2015192_01

Start Time:	2015-192T00:00:02.319	Stop Time:	2015-192T23:59:59.893
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015193_01

Start Time:	2015-193T00:00:05.518	Stop Time:	2015-193T23:59:54.718
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015194_01

Start Time:	2015-194T00:00:00.343	Stop Time:	2015-194T23:59:55.167
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015195_01

Start Time:	2015-195T00:00:00.792	Stop Time:	2015-195T23:59:54.617
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015196_01

Start Time:	2015-196T00:00:00.242	Stop Time:	2015-196T23:59:55.570
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015197_01

Start Time:	2015-197T00:00:01.191	Stop Time:	2015-197T23:59:56.558
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_2015198_01

Start Time:	2015-198T00:00:04.504	Stop Time:	2015-198T23:59:52.266
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_2015199_01

Start Time:	2015-199T00:00:00.246	Stop Time:	2015-199T23:59:59.032
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015200_01

Start Time:	2015-200T00:00:06.918	Stop Time:	2015-200T23:59:57.489
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_2015201_01

Start Time:	2015-201T00:00:03.114	Stop Time:	2015-201T23:59:59.438
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_2015202_01

Start Time:	2015-202T00:00:05.063	Stop Time:	2015-202T23:59:57.763
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015203_01

Start Time:	2015-203T00:00:03.388	Stop Time:	2015-203T23:59:59.337
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015204_01

Start Time:	2015-204T00:00:04.962	Stop Time:	2015-204T23:59:57.538
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015205_01

Start Time:	2015-205T00:00:03.163	Stop Time:	2015-205T23:59:55.862
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015206_01

Start Time:	2015-206T00:00:01.487	Stop Time:	2015-206T23:59:58.311
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015207_01

Start Time:	2015-207T00:00:03.936	Stop Time:	2015-207T23:59:59.511
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015208_01

Start Time:	2015-208T00:00:03.261	Stop Time:	2015-208T23:59:58.675
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015209_01

Start Time:	2015-209T00:00:06.620	Stop Time:	2015-209T23:59:55.785
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015210_01

Start Time:	2015-210T00:00:01.414	Stop Time:	2015-210T23:59:59.984
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015211_01

Start Time:	2015-211T00:00:05.609	Stop Time:	2015-211T23:59:54.809
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015212_01

Start Time:	2015-212T00:00:00.434	Stop Time:	2015-212T23:59:56.258
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015213_01

Start Time:	2015-213T00:00:00.008	Stop Time:	2015-213T23:59:56.708
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_2015214_01

Start Time:	2015-214T00:00:02.333	Stop Time:	2015-214T23:59:56.157
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015215_01

Start Time:	2015-215T00:00:01.782	Stop Time:	2015-215T23:59:56.606
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015216_01

Start Time:	2015-216T00:00:02.231	Stop Time:	2015-216T23:59:57.056
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015217_01

Start Time:	2015-217T00:00:02.681	Stop Time:	2015-217T23:59:52.130
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_2015218_01

Start Time:	2015-218T00:00:00.154	Stop Time:	2015-218T23:59:59.205
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015219_01

Start Time:	2015-219T00:00:04.830	Stop Time:	2015-219T23:59:57.529
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015220_01

Start Time:	2015-220T00:00:03.154	Stop Time:	2015-220T23:59:58.729
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_2015221_01

Start Time:	2015-221T00:00:04.354	Stop Time:	2015-221T23:59:57.303
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_2015222_01

Start Time:	2015-222T00:00:01.053	Stop Time:	2015-222T23:59:56.128
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015223_01

Start Time:	2015-223T00:00:01.753	Stop Time:	2015-223T23:59:55.327
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_2015224_01

Start Time:	2015-224T00:00:00.952	Stop Time:	2015-224T23:59:56.276
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_2015225_01

Start Time:	2015-225T00:00:01.901	Stop Time:	2015-225T23:59:58.601
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015226_01

Start Time:	2015-226T00:00:04.226	Stop Time:	2015-226T23:59:58.925
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015227_01

Start Time:	2015-227T00:00:04.550	Stop Time:	2015-227T23:59:59.000
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_2015228_01

Start Time:	2015-228T00:00:04.625	Stop Time:	2015-228T23:59:59.449
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_2015229_01

Start Time:	2015-229T00:00:05.074	Stop Time:	2015-229T23:59:59.899
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015230_01

Start Time:	2015-230T00:00:05.524	Stop Time:	2015-230T23:59:53.805
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015231_01

Start Time:	2015-231T00:00:01.762	Stop Time:	2015-231T23:59:53.985
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015232_01

Start Time:	2015-232T00:00:01.954	Stop Time:	2015-232T23:59:54.560
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015233_01

Start Time:	2015-233T00:00:01.122	Stop Time:	2015-233T23:59:59.696
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015234_01

Start Time:	2015-234T00:00:06.259	Stop Time:	2015-234T22:01:45.129
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_2015235_01

Start Time:	2015-235T03:09:54.577	Stop Time:	2015-235T23:59:53.689
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_2015236_01

Start Time:	2015-236T00:00:01.658	Stop Time:	2015-236T23:59:59.295
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_2015237_01

Start Time:	2015-237T00:00:07.264	Stop Time:	2015-237T23:59:55.932
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_2015238_01

Start Time:	2015-238T00:00:03.901	Stop Time:	2015-238T23:59:53.069
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015239_01

Start Time:	2015-239T00:00:01.037	Stop Time:	2015-239T23:59:58.674
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015240_01

Start Time:	2015-240T00:00:06.643	Stop Time:	2015-240T23:59:56.311
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015241_01

Start Time:	2015-241T00:00:04.280	Stop Time:	2015-241T23:59:53.448
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015242_01

Start Time:	2015-242T00:00:01.417	Stop Time:	2015-242T23:59:59.054
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015243_01

Start Time:	2015-243T00:00:07.023	Stop Time:	2015-243T23:59:56.695
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015244_01

Start Time:	2015-244T00:00:04.660	Stop Time:	2015-244T23:59:53.828
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015245_01

Start Time:	2015-245T00:00:01.797	Stop Time:	2015-245T23:59:58.434
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015246_01

Start Time:	2015-246T00:00:06.402	Stop Time:	2015-246T23:59:55.758
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_2015247_01

Start Time:	2015-247T00:00:03.727	Stop Time:	2015-247T23:59:53.395
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015248_01

Start Time:	2015-248T00:00:01.364	Stop Time:	2015-248T23:59:56.720
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015249_01

Start Time:	2015-249T00:00:04.688	Stop Time:	2015-249T23:59:56.044
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015250_01

Start Time:	2015-250T00:00:04.013	Stop Time:	2015-250T23:59:58.400
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_2015251_01

Start Time:	2015-251T00:00:06.368	Stop Time:	2015-251T23:59:59.787
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_2015252_01

Start Time:	2015-252T00:00:03.537	Stop Time:	2015-252T23:59:59.361
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_2015253_01

Start Time:	2015-253T00:00:04.986	Stop Time:	2015-253T23:59:56.292
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015254_01

Start Time:	2015-254T00:00:04.390	Stop Time:	2015-254T23:59:57.886
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015255_01

Start Time:	2015-255T00:00:01.636	Stop Time:	2015-255T23:59:54.586
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015256_01

Start Time:	2015-256T00:00:00.210	Stop Time:	2015-256T23:59:55.035
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015257_01

Start Time:	2015-257T00:00:00.660	Stop Time:	2015-257T23:59:54.484
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015258_01

Start Time:	2015-258T00:00:00.109	Stop Time:	2015-258T23:59:54.934
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015259_01

Start Time:	2015-259T00:00:00.559	Stop Time:	2015-259T23:59:54.383
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015260_01

Start Time:	2015-260T00:00:00.008	Stop Time:	2015-260T23:59:54.833
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015261_01

Start Time:	2015-261T00:00:00.458	Stop Time:	2015-261T23:59:55.282
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015262_01

Start Time:	2015-262T00:00:00.907	Stop Time:	2015-262T23:59:58.482
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015263_01

Start Time:	2015-263T00:00:04.107	Stop Time:	2015-263T23:59:58.931
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_2015264_01

Start Time:	2015-264T00:00:04.556	Stop Time:	2015-264T23:59:59.374
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015265_01

Start Time:	2015-265T00:00:07.393	Stop Time:	2015-265T23:59:55.675
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015266_01

Start Time:	2015-266T00:00:01.300	Stop Time:	2015-266T23:59:54.210
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015267_01

Start Time:	2015-267T00:00:02.230	Stop Time:	2015-267T23:59:58.949
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_2015268_01

Start Time:	2015-268T00:00:04.578	Stop Time:	2015-268T23:59:56.524
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_2015269_01

Start Time:	2015-269T00:00:02.149	Stop Time:	2015-269T23:59:55.348
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015270_01

Start Time:	2015-270T00:00:00.973	Stop Time:	2015-270T23:59:53.927
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015271_01

Start Time:	2015-271T00:00:01.892	Stop Time:	2015-271T23:59:58.122
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_2015272_01

Start Time:	2015-272T00:00:06.091	Stop Time:	2015-272T23:59:54.826
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015273_01

Start Time:	2015-273T00:00:02.791	Stop Time:	2015-273T23:59:55.772
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015274_01

Start Time:	2015-274T00:00:01.397	Stop Time:	2015-274T23:59:56.428
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015275_01

Start Time:	2015-275T00:00:03.725	Stop Time:	2015-275T23:59:59.546
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_2015276_01

Start Time:	2015-276T00:00:05.175	Stop Time:	2015-276T23:59:59.121
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015277_01

Start Time:	2015-277T00:00:04.745	Stop Time:	2015-277T23:59:58.570
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015278_01

Start Time:	2015-278T00:00:04.195	Stop Time:	2015-278T23:59:53.485
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015279_01

Start Time:	2015-279T00:00:01.465	Stop Time:	2015-279T23:59:53.532
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_2015280_01

Start Time:	2015-280T00:00:01.501	Stop Time:	2015-280T23:59:58.892
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_2015281_01

Start Time:	2015-281T00:00:06.845	Stop Time:	2015-281T23:59:53.986
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015282_01

Start Time:	2015-282T00:00:01.873	Stop Time:	2015-282T23:59:53.881
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015283_01

Start Time:	2015-283T00:00:01.849	Stop Time:	2015-283T23:59:53.803
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_2015284_01

Start Time:	2015-284T00:00:01.838	Stop Time:	2015-284T23:59:56.842
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_2015285_01

Start Time:	2015-285T00:00:04.811	Stop Time:	2015-285T23:59:57.167
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015286_01

Start Time:	2015-286T00:00:02.792	Stop Time:	2015-286T23:59:56.617
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015287_01

Start Time:	2015-287T00:00:02.242	Stop Time:	2015-287T23:59:58.504
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015288_01

Start Time:	2015-288T00:00:06.496	Stop Time:	2015-288T23:59:59.020
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015289_01

Start Time:	2015-289T00:00:06.985	Stop Time:	2015-289T23:59:59.469
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015290_01

Start Time:	2015-290T00:00:03.216	Stop Time:	2015-290T23:59:55.290
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015291_01

Start Time:	2015-291T00:00:00.919	Stop Time:	2015-291T23:59:59.490
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015292_01

Start Time:	2015-292T00:00:05.115	Stop Time:	2015-292T23:59:55.740
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015293_01

Start Time:	2015-293T00:00:03.736	Stop Time:	2015-293T23:59:56.209
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015294_01

Start Time:	2015-294T00:00:04.194	Stop Time:	2015-294T23:59:55.464
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015295_01

Start Time:	2015-295T00:00:01.089	Stop Time:	2015-295T23:59:57.070
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015296_01

Start Time:	2015-296T00:00:05.167	Stop Time:	2015-296T23:59:57.527
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015297_01

Start Time:	2015-297T00:00:05.484	Stop Time:	2015-297T23:59:53.067
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015298_01

Start Time:	2015-298T00:00:01.059	Stop Time:	2015-298T23:59:56.481
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015299_01

Start Time:	2015-299T00:00:04.450	Stop Time:	2015-299T23:59:57.087
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_2015300_01

Start Time:	2015-300T00:00:02.712	Stop Time:	2015-300T23:59:59.411
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015301_01

Start Time:	2015-301T00:00:03.161	Stop Time:	2015-301T23:59:58.978
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015302_01

Start Time:	2015-302T00:00:06.865	Stop Time:	2015-302T23:59:57.740
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015303_01

Start Time:	2015-303T00:00:05.686	Stop Time:	2015-303T23:59:58.542
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015304_01

Start Time:	2015-304T00:00:06.522	Stop Time:	2015-304T23:59:54.522
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_2015305_01

Start Time:	2015-305T00:00:02.213	Stop Time:	2015-305T23:59:57.784
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015306_01

Start Time:	2015-306T00:00:03.409	Stop Time:	2015-306T23:59:59.358
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_2015307_01

Start Time:	2015-307T00:00:04.983	Stop Time:	2015-307T23:59:54.808
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_2015308_01

Start Time:	2015-308T00:00:00.433	Stop Time:	2015-308T23:59:52.011
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015309_01

Start Time:	2015-309T00:00:00.097	Stop Time:	2015-309T23:59:53.461
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_2015310_01

Start Time:	2015-310T00:00:01.481	Stop Time:	2015-310T23:59:59.282
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015311_01

Start Time:	2015-311T00:00:04.907	Stop Time:	2015-311T20:16:03.817
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_2015312_01

Start Time:	2015-312T08:22:35.168	Stop Time:	2015-312T23:59:56.806
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_2015313_01

Start Time:	2015-313T00:00:02.431	Stop Time:	2015-313T23:59:56.342
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015314_01

Start Time:	2015-314T00:00:04.349	Stop Time:	2015-314T23:59:58.518
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015315_01

Start Time:	2015-315T00:00:06.588	Stop Time:	2015-315T23:59:57.460
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015316_01

Start Time:	2015-316T00:00:05.495	Stop Time:	2015-316T23:59:54.855
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015317_01

Start Time:	2015-317T00:00:00.480	Stop Time:	2015-317T23:59:59.011
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015318_01

Start Time:	2015-318T00:00:07.007	Stop Time:	2015-318T23:59:57.629
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_2015319_01

Start Time:	2015-319T00:00:03.254	Stop Time:	2015-319T23:59:58.203
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015320_01

Start Time:	2015-320T00:00:03.828	Stop Time:	2015-320T23:59:55.778
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015321_01

Start Time:	2015-321T00:00:01.407	Stop Time:	2015-321T23:59:59.978
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015322_01

Start Time:	2015-322T00:00:05.603	Stop Time:	2015-322T23:59:53.427
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015323_01

Start Time:	2015-323T00:00:01.451	Stop Time:	2015-323T23:59:58.877
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_2015324_01

Start Time:	2015-324T00:00:04.502	Stop Time:	2015-324T23:59:54.952
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015325_01

Start Time:	2015-325T00:00:00.577	Stop Time:	2015-325T23:59:57.655
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_2015326_01

Start Time:	2015-326T00:00:03.276	Stop Time:	2015-326T23:59:54.851
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015327_01

Start Time:	2015-327T00:00:00.476	Stop Time:	2015-327T23:59:59.051
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015328_01

Start Time:	2015-328T00:00:02.801	Stop Time:	2015-328T19:25:30.480
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015329_01

Start Time:	2015-329T05:46:23.872	Stop Time:	2015-329T23:59:58.914
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015330_01

Start Time:	2015-330T00:00:05.476	Stop Time:	2015-330T23:59:56.300
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015331_01

Start Time:	2015-331T00:00:01.867	Stop Time:	2015-331T23:59:59.625
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015332_01

Start Time:	2015-332T00:00:06.187	Stop Time:	2015-332T23:59:57.386
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015333_01

Start Time:	2015-333T00:00:03.949	Stop Time:	2015-333T23:59:54.148
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015334_01

Start Time:	2015-334T00:00:00.710	Stop Time:	2015-334T23:59:54.660
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_2015335_01

Start Time:	2015-335T00:00:00.285	Stop Time:	2015-335T23:59:55.109
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015336_01

Start Time:	2015-336T00:00:00.734	Stop Time:	2015-336T23:59:54.558
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_2015337_01

Start Time:	2015-337T00:00:00.183	Stop Time:	2015-337T23:59:58.757
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015338_01

Start Time:	2015-338T00:00:04.382	Stop Time:	2015-338T23:59:55.273
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_2015339_01

Start Time:	2015-339T00:00:03.257	Stop Time:	2015-339T23:59:57.905
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015340_01

Start Time:	2015-340T00:00:03.530	Stop Time:	2015-340T23:59:54.667
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015341_01

Start Time:	2015-341T00:00:01.229	Stop Time:	2015-341T23:59:56.554
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015342_01

Start Time:	2015-342T00:00:00.303	Stop Time:	2015-342T23:59:58.835
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015343_01

Start Time:	2015-343T00:00:06.764	Stop Time:	2015-343T23:59:58.264
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015344_01

Start Time:	2015-344T00:00:04.827	Stop Time:	2015-344T23:59:55.026
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_2015345_01

Start Time:	2015-345T00:00:01.588	Stop Time:	2015-345T23:59:58.350
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015346_01

Start Time:	2015-346T00:00:04.913	Stop Time:	2015-346T23:59:55.112
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_2015347_01

Start Time:	2015-347T00:00:01.674	Stop Time:	2015-347T23:59:55.248
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015348_01

Start Time:	2015-348T00:00:00.873	Stop Time:	2015-348T23:59:55.697
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_2015349_01

Start Time:	2015-349T00:00:01.322	Stop Time:	2015-349T23:59:55.147
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015350_01

Start Time:	2015-350T00:00:00.772	Stop Time:	2015-350T23:59:55.596
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015351_01

Start Time:	2015-351T00:00:01.221	Stop Time:	2015-351T23:59:56.044
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015352_01

Start Time:	2015-352T00:00:01.669	Stop Time:	2015-352T23:59:55.493
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015353_01

Start Time:	2015-353T00:00:01.118	Stop Time:	2015-353T23:59:56.942
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015354_01

Start Time:	2015-354T00:00:02.567	Stop Time:	2015-354T23:59:55.368
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015355_01

Start Time:	2015-355T00:00:03.645	Stop Time:	2015-355T23:59:59.840
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015356_01

Start Time:	2015-356T00:00:05.465	Stop Time:	2015-356T23:59:59.290
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015357_01

Start Time:	2015-357T00:00:04.915	Stop Time:	2015-357T23:59:55.114
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015358_01

Start Time:	2015-358T00:00:00.739	Stop Time:	2015-358T23:59:54.563
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015359_01

Start Time:	2015-359T00:00:00.188	Stop Time:	2015-359T23:59:55.012
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_2015360_01

Start Time:	2015-360T00:00:00.637	Stop Time:	2015-360T23:59:58.086
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015361_01

Start Time:	2015-361T00:00:01.836	Stop Time:	2015-361T23:59:55.035
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015362_01

Start Time:	2015-362T00:00:00.660	Stop Time:	2015-362T23:59:56.484
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015363_01

Start Time:	2015-363T00:00:02.109	Stop Time:	2015-363T23:59:58.059
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2015364_01

Start Time:	2015-364T00:00:03.687	Stop Time:	2015-364T23:59:55.633
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_2015365_01

Start Time:	2015-365T00:00:01.258	Stop Time:	2015-365T23:59:57.082
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric 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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