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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

This contains calibrated Saturn tour data collected by the LEMMS sensor of the MIMI instrument aboard the Cassini spacecraft for the Cassini mission.

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/ 2014 /

LACCFULL0_2014001_01

Start Time:	2014-001T00:00:01.148	Stop Time:	2014-001T23:59:59.787
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_2014002_01

Start Time:	2014-002T00:00:03.541	Stop Time:	2014-002T23:59:58.488
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014003_01

Start Time:	2014-003T00:00:05.050	Stop Time:	2014-003T23:59:58.939
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014004_01

Start Time:	2014-004T00:00:04.564	Stop Time:	2014-004T23:59:59.390
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014005_01

Start Time:	2014-005T00:00:05.015	Stop Time:	2014-005T23:59:58.841
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014006_01

Start Time:	2014-006T00:00:04.466	Stop Time:	2014-006T23:59:57.667
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_2014007_01

Start Time:	2014-007T00:00:03.292	Stop Time:	2014-007T23:59:55.118
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014008_01

Start Time:	2014-008T00:00:03.086	Stop Time:	2014-008T23:59:53.698
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014009_01

Start Time:	2014-009T00:00:01.612	Stop Time:	2014-009T23:59:54.070
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_2014010_01

Start Time:	2014-010T00:00:01.988	Stop Time:	2014-010T22:28:46.068
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014011_01

Start Time:	2014-011T12:03:40.323	Stop Time:	2014-011T23:59:58.796
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014012_01

Start Time:	2014-012T00:00:02.546	Stop Time:	2014-012T23:59:58.310
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014013_01

Start Time:	2014-013T00:00:04.872	Stop Time:	2014-013T23:59:56.948
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_2014014_01

Start Time:	2014-014T00:00:00.698	Stop Time:	2014-014T23:59:58.712
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014015_01

Start Time:	2014-015T00:00:05.274	Stop Time:	2014-015T23:59:55.475
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014016_01

Start Time:	2014-016T00:00:02.038	Stop Time:	2014-016T23:59:55.551
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014017_01

Start Time:	2014-017T00:00:02.114	Stop Time:	2014-017T23:59:59.877
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_2014018_01

Start Time:	2014-018T00:00:06.440	Stop Time:	2014-018T23:59:58.770
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014019_01

Start Time:	2014-019T00:00:07.207	Stop Time:	2014-019T23:59:57.404
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014020_01

Start Time:	2014-020T00:00:03.967	Stop Time:	2014-020T23:59:56.980
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014021_01

Start Time:	2014-021T00:00:02.605	Stop Time:	2014-021T23:59:56.430
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014022_01

Start Time:	2014-022T00:00:02.055	Stop Time:	2014-022T23:59:56.881
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_2014023_01

Start Time:	2014-023T00:00:02.506	Stop Time:	2014-023T23:59:57.332
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014024_01

Start Time:	2014-024T00:00:02.957	Stop Time:	2014-024T23:59:56.783
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014025_01

Start Time:	2014-025T00:00:02.408	Stop Time:	2014-025T23:59:57.234
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014026_01

Start Time:	2014-026T00:00:02.859	Stop Time:	2014-026T23:59:57.685
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014027_01

Start Time:	2014-027T00:00:03.310	Stop Time:	2014-027T23:59:55.761
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014028_01

Start Time:	2014-028T00:00:01.386	Stop Time:	2014-028T23:59:58.087
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_2014029_01

Start Time:	2014-029T00:00:03.715	Stop Time:	2014-029T23:59:59.913
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_2014030_01

Start Time:	2014-030T00:00:05.537	Stop Time:	2014-030T23:59:56.863
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014031_01

Start Time:	2014-031T00:00:02.488	Stop Time:	2014-031T23:59:57.439
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014032_01

Start Time:	2014-032T00:00:03.068	Stop Time:	2014-032T23:59:57.265
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014033_01

Start Time:	2014-033T00:00:02.890	Stop Time:	2014-033T23:59:55.841
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014034_01

Start Time:	2014-034T00:00:01.466	Stop Time:	2014-034T23:59:54.417
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014035_01

Start Time:	2014-035T00:00:00.042	Stop Time:	2014-035T23:59:53.993
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014036_01

Start Time:	2014-036T00:00:00.556	Stop Time:	2014-036T23:59:59.194
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014037_01

Start Time:	2014-037T00:00:04.819	Stop Time:	2014-037T23:59:57.770
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014038_01

Start Time:	2014-038T00:00:01.520	Stop Time:	2014-038T23:59:57.346
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_2014039_01

Start Time:	2014-039T00:00:02.971	Stop Time:	2014-039T23:59:57.797
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014040_01

Start Time:	2014-040T00:00:03.422	Stop Time:	2014-040T23:59:59.123
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_2014041_01

Start Time:	2014-041T00:00:02.873	Stop Time:	2014-041T23:59:56.824
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014042_01

Start Time:	2014-042T00:00:00.574	Stop Time:	2014-042T23:59:58.275
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014043_01

Start Time:	2014-043T00:00:02.025	Stop Time:	2014-043T23:59:55.851
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_2014044_01

Start Time:	2014-044T00:00:01.476	Stop Time:	2014-044T23:59:58.177
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014045_01

Start Time:	2014-045T00:00:01.927	Stop Time:	2014-045T23:59:56.753
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014046_01

Start Time:	2014-046T00:00:02.378	Stop Time:	2014-046T23:59:56.704
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014047_01

Start Time:	2014-047T00:00:02.329	Stop Time:	2014-047T23:59:59.030
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_2014048_01

Start Time:	2014-048T00:00:04.655	Stop Time:	2014-048T23:59:59.855
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_2014049_01

Start Time:	2014-049T00:00:05.480	Stop Time:	2014-049T23:59:55.185
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014050_01

Start Time:	2014-050T00:00:00.806	Stop Time:	2014-050T23:59:54.636
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014051_01

Start Time:	2014-051T00:00:00.257	Stop Time:	2014-051T23:59:58.583
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014052_01

Start Time:	2014-052T00:00:04.208	Stop Time:	2014-052T23:59:58.034
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014053_01

Start Time:	2014-053T00:00:03.659	Stop Time:	2014-053T23:59:58.360
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014054_01

Start Time:	2014-054T00:00:03.985	Stop Time:	2014-054T23:59:58.811
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014055_01

Start Time:	2014-055T00:00:04.436	Stop Time:	2014-055T23:59:58.137
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014056_01

Start Time:	2014-056T00:00:03.762	Stop Time:	2014-056T23:59:58.588
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014057_01

Start Time:	2014-057T00:00:04.213	Stop Time:	2014-057T23:59:58.039
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014058_01

Start Time:	2014-058T00:00:03.664	Stop Time:	2014-058T23:59:58.490
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_2014059_01

Start Time:	2014-059T00:00:04.115	Stop Time:	2014-059T23:59:58.941
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014060_01

Start Time:	2014-060T00:00:04.566	Stop Time:	2014-060T23:59:58.392
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014061_01

Start Time:	2014-061T00:00:04.017	Stop Time:	2014-061T23:59:55.468
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014062_01

Start Time:	2014-062T00:00:01.093	Stop Time:	2014-062T23:59:57.919
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014063_01

Start Time:	2014-063T00:00:03.544	Stop Time:	2014-063T23:59:59.745
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_2014064_01

Start Time:	2014-064T00:00:05.370	Stop Time:	2014-064T23:59:58.321
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014065_01

Start Time:	2014-065T00:00:04.883	Stop Time:	2014-065T23:59:59.771
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014066_01

Start Time:	2014-066T00:00:05.400	Stop Time:	2014-066T23:59:58.347
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014067_01

Start Time:	2014-067T00:00:03.972	Stop Time:	2014-067T23:59:58.798
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_2014068_01

Start Time:	2014-068T00:00:02.548	Stop Time:	2014-068T23:59:59.873
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014069_01

Start Time:	2014-069T00:00:05.498	Stop Time:	2014-069T23:59:58.949
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_2014070_01

Start Time:	2014-070T00:00:05.512	Stop Time:	2014-070T23:59:54.525
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014071_01

Start Time:	2014-071T00:00:01.088	Stop Time:	2014-071T23:59:57.851
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_2014072_01

Start Time:	2014-072T00:00:04.414	Stop Time:	2014-072T23:59:57.427
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_2014073_01

Start Time:	2014-073T00:00:05.396	Stop Time:	2014-073T23:59:54.565
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014074_01

Start Time:	2014-074T00:00:02.534	Stop Time:	2014-074T23:59:53.110
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_2014075_01

Start Time:	2014-075T00:00:01.079	Stop Time:	2014-075T23:59:58.717
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014076_01

Start Time:	2014-076T00:00:06.686	Stop Time:	2014-076T23:59:56.360
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014077_01

Start Time:	2014-077T00:00:04.324	Stop Time:	2014-077T23:59:53.494
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014078_01

Start Time:	2014-078T00:00:01.463	Stop Time:	2014-078T23:59:59.101
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014079_01

Start Time:	2014-079T00:00:07.070	Stop Time:	2014-079T23:59:56.240
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014080_01

Start Time:	2014-080T00:00:04.712	Stop Time:	2014-080T23:59:53.878
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014081_01

Start Time:	2014-081T00:00:01.847	Stop Time:	2014-081T23:59:59.485
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_2014082_01

Start Time:	2014-082T00:00:07.454	Stop Time:	2014-082T23:59:58.905
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_2014083_01

Start Time:	2014-083T00:00:06.874	Stop Time:	2014-083T23:59:57.043
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014084_01

Start Time:	2014-084T00:00:04.516	Stop Time:	2014-084T23:59:57.494
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014085_01

Start Time:	2014-085T00:00:04.967	Stop Time:	2014-085T23:59:55.133
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_2014086_01

Start Time:	2014-086T00:00:03.102	Stop Time:	2014-086T23:59:56.584
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_2014087_01

Start Time:	2014-087T00:00:04.552	Stop Time:	2014-087T23:59:54.222
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014088_01

Start Time:	2014-088T00:00:02.191	Stop Time:	2014-088T23:59:58.673
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014089_01

Start Time:	2014-089T00:00:06.642	Stop Time:	2014-089T23:59:59.089
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014090_01

Start Time:	2014-090T00:00:07.175	Stop Time:	2014-090T23:59:58.325
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014091_01

Start Time:	2014-091T00:00:06.294	Stop Time:	2014-091T23:59:54.870
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014092_01

Start Time:	2014-092T00:00:02.838	Stop Time:	2014-092T23:59:54.289
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014093_01

Start Time:	2014-093T00:00:02.258	Stop Time:	2014-093T23:59:58.771
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014094_01

Start Time:	2014-094T00:00:06.740	Stop Time:	2014-094T23:59:54.035
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_2014095_01

Start Time:	2014-095T00:00:02.004	Stop Time:	2014-095T23:59:52.927
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_2014096_01

Start Time:	2014-096T00:00:00.892	Stop Time:	2014-096T23:59:58.999
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014097_01

Start Time:	2014-097T00:00:04.624	Stop Time:	2014-097T23:59:57.575
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014098_01

Start Time:	2014-098T00:00:01.325	Stop Time:	2014-098T23:59:55.276
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_2014099_01

Start Time:	2014-099T00:00:00.901	Stop Time:	2014-099T23:59:59.477
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014100_01

Start Time:	2014-100T00:00:03.227	Stop Time:	2014-100T23:59:58.678
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014101_01

Start Time:	2014-101T00:00:02.428	Stop Time:	2014-101T23:59:56.004
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014102_01

Start Time:	2014-102T00:00:01.629	Stop Time:	2014-102T23:59:58.330
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014103_01

Start Time:	2014-103T00:00:02.080	Stop Time:	2014-103T23:59:59.781
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_2014104_01

Start Time:	2014-104T00:00:03.531	Stop Time:	2014-104T23:59:58.232
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014105_01

Start Time:	2014-105T00:00:03.857	Stop Time:	2014-105T23:59:58.682
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014106_01

Start Time:	2014-106T00:00:04.307	Stop Time:	2014-106T23:59:59.887
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014107_01

Start Time:	2014-107T00:00:05.508	Stop Time:	2014-107T23:59:54.709
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014108_01

Start Time:	2014-108T00:00:00.338	Stop Time:	2014-108T12:37:33.420
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014109_01

Start Time:	2014-109T01:01:41.766	Stop Time:	2014-109T23:59:58.986
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_2014110_01

Start Time:	2014-110T00:00:04.611	Stop Time:	2014-110T23:59:55.562
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014111_01

Start Time:	2014-111T00:00:01.187	Stop Time:	2014-111T23:59:55.513
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014112_01

Start Time:	2014-112T00:00:01.138	Stop Time:	2014-112T23:59:57.593
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014113_01

Start Time:	2014-113T00:00:03.214	Stop Time:	2014-113T23:59:54.665
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014114_01

Start Time:	2014-114T00:00:00.290	Stop Time:	2014-114T23:59:55.991
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014115_01

Start Time:	2014-115T00:00:01.616	Stop Time:	2014-115T23:59:56.817
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014116_01

Start Time:	2014-116T00:00:02.442	Stop Time:	2014-116T23:59:56.268
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014117_01

Start Time:	2014-117T00:00:01.893	Stop Time:	2014-117T23:59:57.593
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014118_01

Start Time:	2014-118T00:00:03.218	Stop Time:	2014-118T23:59:57.044
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_2014119_01

Start Time:	2014-119T00:00:02.669	Stop Time:	2014-119T23:59:54.996
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_2014120_01

Start Time:	2014-120T00:00:00.621	Stop Time:	2014-120T23:59:55.447
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014121_01

Start Time:	2014-121T00:00:01.072	Stop Time:	2014-121T23:59:59.898
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014122_01

Start Time:	2014-122T00:00:05.523	Stop Time:	2014-122T23:59:59.349
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014123_01

Start Time:	2014-123T00:00:04.974	Stop Time:	2014-123T23:59:59.800
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014124_01

Start Time:	2014-124T00:00:05.425	Stop Time:	2014-124T23:59:54.626
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014125_01

Start Time:	2014-125T00:00:00.251	Stop Time:	2014-125T23:59:59.702
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014126_01

Start Time:	2014-126T00:00:05.327	Stop Time:	2014-126T23:59:54.528
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014127_01

Start Time:	2014-127T00:00:00.153	Stop Time:	2014-127T11:18:27.019
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014129_01

Start Time:	2014-129T10:54:34.559	Stop Time:	2014-129T23:59:54.880
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_2014130_01

Start Time:	2014-130T00:00:00.505	Stop Time:	2014-130T23:59:59.956
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014131_01

Start Time:	2014-131T00:00:05.581	Stop Time:	2014-131T23:59:54.782
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014132_01

Start Time:	2014-132T00:00:00.407	Stop Time:	2014-132T23:59:55.233
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014133_01

Start Time:	2014-133T00:00:00.858	Stop Time:	2014-133T23:59:56.559
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014134_01

Start Time:	2014-134T00:00:02.184	Stop Time:	2014-134T23:59:57.010
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_2014135_01

Start Time:	2014-135T00:00:02.635	Stop Time:	2014-135T23:59:57.461
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014136_01

Start Time:	2014-136T00:00:03.086	Stop Time:	2014-136T23:59:59.787
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_2014137_01

Start Time:	2014-137T00:00:05.416	Stop Time:	2014-137T23:59:58.363
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014138_01

Start Time:	2014-138T00:00:03.988	Stop Time:	2014-138T23:59:57.813
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014139_01

Start Time:	2014-139T00:00:03.438	Stop Time:	2014-139T23:59:57.764
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_2014140_01

Start Time:	2014-140T00:00:03.389	Stop Time:	2014-140T23:59:59.215
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014141_01

Start Time:	2014-141T00:00:02.965	Stop Time:	2014-141T23:59:58.791
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014142_01

Start Time:	2014-142T00:00:04.416	Stop Time:	2014-142T23:59:57.742
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014143_01

Start Time:	2014-143T00:00:03.367	Stop Time:	2014-143T23:59:58.193
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014144_01

Start Time:	2014-144T00:00:03.818	Stop Time:	2014-144T23:59:57.644
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_2014145_01

Start Time:	2014-145T00:00:03.269	Stop Time:	2014-145T23:59:58.095
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_2014146_01

Start Time:	2014-146T00:00:03.720	Stop Time:	2014-146T23:59:58.546
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_2014147_01

Start Time:	2014-147T00:00:04.171	Stop Time:	2014-147T23:59:57.997
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_2014148_01

Start Time:	2014-148T00:00:03.622	Stop Time:	2014-148T23:59:58.447
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014149_01

Start Time:	2014-149T00:00:04.072	Stop Time:	2014-149T23:59:58.898
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014150_01

Start Time:	2014-150T00:00:04.523	Stop Time:	2014-150T23:59:58.349
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014151_01

Start Time:	2014-151T00:00:03.974	Stop Time:	2014-151T23:59:58.800
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014152_01

Start Time:	2014-152T00:00:04.425	Stop Time:	2014-152T23:59:59.251
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014153_01

Start Time:	2014-153T00:00:04.876	Stop Time:	2014-153T23:59:58.702
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014154_01

Start Time:	2014-154T00:00:04.327	Stop Time:	2014-154T23:59:59.153
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014155_01

Start Time:	2014-155T00:00:04.778	Stop Time:	2014-155T23:59:56.229
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_2014156_01

Start Time:	2014-156T00:00:01.854	Stop Time:	2014-156T23:59:56.680
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014157_01

Start Time:	2014-157T00:00:02.305	Stop Time:	2014-157T23:59:56.881
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_2014158_01

Start Time:	2014-158T00:00:02.506	Stop Time:	2014-158T23:59:56.331
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014159_01

Start Time:	2014-159T00:00:01.956	Stop Time:	2014-159T23:59:59.032
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_2014160_01

Start Time:	2014-160T00:00:04.657	Stop Time:	2014-160T23:59:59.483
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014161_01

Start Time:	2014-161T00:00:05.108	Stop Time:	2014-161T23:59:55.059
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_2014162_01

Start Time:	2014-162T00:00:00.684	Stop Time:	2014-162T23:59:55.510
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_2014163_01

Start Time:	2014-163T00:00:01.135	Stop Time:	2014-163T23:59:57.336
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_2014164_01

Start Time:	2014-164T00:00:02.961	Stop Time:	2014-164T23:59:54.662
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014165_01

Start Time:	2014-165T00:00:00.287	Stop Time:	2014-165T23:59:58.738
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014166_01

Start Time:	2014-166T00:00:04.363	Stop Time:	2014-166T23:59:58.189
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014167_01

Start Time:	2014-167T00:00:03.814	Stop Time:	2014-167T23:59:58.640
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014168_01

Start Time:	2014-168T00:00:02.393	Stop Time:	2014-168T23:59:59.091
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_2014169_01

Start Time:	2014-169T00:00:04.716	Stop Time:	2014-169T23:59:59.493
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_2014170_01

Start Time:	2014-170T00:00:05.118	Stop Time:	2014-170T23:59:59.943
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014171_01

Start Time:	2014-171T00:00:03.693	Stop Time:	2014-171T23:59:54.769
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014172_01

Start Time:	2014-172T00:00:00.394	Stop Time:	2014-172T23:59:58.969
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014173_01

Start Time:	2014-173T00:00:04.598	Stop Time:	2014-173T23:59:59.419
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014174_01

Start Time:	2014-174T00:00:05.048	Stop Time:	2014-174T23:59:58.870
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014175_01

Start Time:	2014-175T00:00:04.499	Stop Time:	2014-175T23:59:59.320
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014176_01

Start Time:	2014-176T00:00:04.949	Stop Time:	2014-176T23:59:58.771
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014177_01

Start Time:	2014-177T00:00:04.399	Stop Time:	2014-177T23:59:59.221
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014178_01

Start Time:	2014-178T00:00:04.850	Stop Time:	2014-178T23:59:59.671
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014179_01

Start Time:	2014-179T00:00:05.300	Stop Time:	2014-179T23:59:58.770
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014180_01

Start Time:	2014-180T00:00:06.790	Stop Time:	2014-180T23:59:55.697
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_2014181_01

Start Time:	2014-181T00:00:01.322	Stop Time:	2014-181T23:59:59.159
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014182_01

Start Time:	2014-182T00:00:07.089	Stop Time:	2014-182T23:59:52.469
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_2014183_01

Start Time:	2014-183T00:00:00.539	Stop Time:	2014-183T23:59:57.822
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014184_01

Start Time:	2014-184T00:00:05.853	Stop Time:	2014-184T23:59:56.424
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014185_01

Start Time:	2014-185T00:00:04.471	Stop Time:	2014-185T23:59:55.406
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014186_01

Start Time:	2014-186T00:00:03.402	Stop Time:	2014-186T23:59:56.102
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014187_01

Start Time:	2014-187T00:00:04.138	Stop Time:	2014-187T23:59:54.600
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014188_01

Start Time:	2014-188T00:00:00.225	Stop Time:	2014-188T23:59:55.925
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_2014189_01

Start Time:	2014-189T00:00:01.550	Stop Time:	2014-189T23:59:55.376
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014190_01

Start Time:	2014-190T00:00:01.000	Stop Time:	2014-190T23:59:55.826
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_2014191_01

Start Time:	2014-191T00:00:01.451	Stop Time:	2014-191T23:59:55.276
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_2014192_01

Start Time:	2014-192T00:00:00.901	Stop Time:	2014-192T23:59:55.727
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_2014193_01

Start Time:	2014-193T00:00:01.352	Stop Time:	2014-193T23:59:56.177
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014194_01

Start Time:	2014-194T00:00:01.802	Stop Time:	2014-194T23:59:58.627
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014195_01

Start Time:	2014-195T00:00:04.252	Stop Time:	2014-195T23:59:58.453
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_2014196_01

Start Time:	2014-196T00:00:04.078	Stop Time:	2014-196T23:59:58.903
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014197_01

Start Time:	2014-197T00:00:04.528	Stop Time:	2014-197T23:59:58.353
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014198_01

Start Time:	2014-198T00:00:03.978	Stop Time:	2014-198T23:59:56.804
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014199_01

Start Time:	2014-199T00:00:00.554	Stop Time:	2014-199T23:59:57.754
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014200_01

Start Time:	2014-200T00:00:01.504	Stop Time:	2014-200T23:59:57.205
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_2014201_01

Start Time:	2014-201T00:00:02.830	Stop Time:	2014-201T23:59:57.655
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_2014202_01

Start Time:	2014-202T00:00:03.280	Stop Time:	2014-202T23:59:58.105
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014203_01

Start Time:	2014-203T00:00:03.730	Stop Time:	2014-203T23:59:55.560
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_2014204_01

Start Time:	2014-204T00:00:03.564	Stop Time:	2014-204T23:59:57.632
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014205_01

Start Time:	2014-205T00:00:03.257	Stop Time:	2014-205T23:59:56.583
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014206_01

Start Time:	2014-206T00:00:02.207	Stop Time:	2014-206T23:59:57.033
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014207_01

Start Time:	2014-207T00:00:02.658	Stop Time:	2014-207T23:59:57.483
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014208_01

Start Time:	2014-208T00:00:03.108	Stop Time:	2014-208T23:59:56.934
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_2014209_01

Start Time:	2014-209T00:00:02.559	Stop Time:	2014-209T23:59:56.466
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014210_01

Start Time:	2014-210T00:00:04.489	Stop Time:	2014-210T23:59:59.334
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014211_01

Start Time:	2014-211T00:00:04.959	Stop Time:	2014-211T23:59:59.785
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_2014212_01

Start Time:	2014-212T00:00:05.410	Stop Time:	2014-212T23:59:54.614
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014213_01

Start Time:	2014-213T00:00:00.235	Stop Time:	2014-213T23:59:59.686
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_2014214_01

Start Time:	2014-214T00:00:05.310	Stop Time:	2014-214T23:59:54.515
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014215_01

Start Time:	2014-215T00:00:00.136	Stop Time:	2014-215T23:59:54.965
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014216_01

Start Time:	2014-216T00:00:00.586	Stop Time:	2014-216T23:59:54.416
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014217_01

Start Time:	2014-217T00:00:00.037	Stop Time:	2014-217T23:59:54.866
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014218_01

Start Time:	2014-218T00:00:00.487	Stop Time:	2014-218T23:59:55.316
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_2014219_01

Start Time:	2014-219T00:00:00.937	Stop Time:	2014-219T23:59:54.767
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014220_01

Start Time:	2014-220T00:00:00.388	Stop Time:	2014-220T23:59:55.217
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014221_01

Start Time:	2014-221T00:00:00.838	Stop Time:	2014-221T23:59:56.414
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014222_01

Start Time:	2014-222T00:00:02.039	Stop Time:	2014-222T23:59:55.864
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014223_01

Start Time:	2014-223T00:00:01.489	Stop Time:	2014-223T23:59:56.314
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014224_01

Start Time:	2014-224T00:00:01.939	Stop Time:	2014-224T23:59:54.284
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_2014225_01

Start Time:	2014-225T00:00:02.308	Stop Time:	2014-225T23:59:57.215
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014226_01

Start Time:	2014-226T00:00:02.840	Stop Time:	2014-226T23:59:57.665
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014227_01

Start Time:	2014-227T00:00:03.290	Stop Time:	2014-227T23:59:58.116
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014228_01

Start Time:	2014-228T00:00:03.741	Stop Time:	2014-228T23:59:55.816
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014229_01

Start Time:	2014-229T00:00:01.441	Stop Time:	2014-229T23:59:55.392
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014230_01

Start Time:	2014-230T00:00:01.017	Stop Time:	2014-230T23:59:55.842
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_2014231_01

Start Time:	2014-231T00:00:01.467	Stop Time:	2014-231T23:59:54.417
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014232_01

Start Time:	2014-232T00:00:00.042	Stop Time:	2014-232T23:59:59.524
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014233_01

Start Time:	2014-233T00:00:07.493	Stop Time:	2014-233T23:59:59.943
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014234_01

Start Time:	2014-234T00:00:05.568	Stop Time:	2014-234T23:59:54.331
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014235_01

Start Time:	2014-235T00:00:02.300	Stop Time:	2014-235T23:59:52.563
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_2014236_01

Start Time:	2014-236T00:00:00.531	Stop Time:	2014-236T23:59:54.294
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014237_01

Start Time:	2014-237T00:00:02.263	Stop Time:	2014-237T23:59:55.526
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014238_01

Start Time:	2014-238T00:00:03.495	Stop Time:	2014-238T23:59:52.289
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014239_01

Start Time:	2014-239T00:00:00.258	Stop Time:	2014-239T23:59:58.395
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_2014240_01

Start Time:	2014-240T00:00:06.364	Stop Time:	2014-240T23:59:55.033
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014241_01

Start Time:	2014-241T00:00:03.002	Stop Time:	2014-241T23:59:55.296
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014242_01

Start Time:	2014-242T00:00:03.265	Stop Time:	2014-242T23:59:52.934
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_2014243_01

Start Time:	2014-243T00:00:00.903	Stop Time:	2014-243T23:59:59.166
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014244_01

Start Time:	2014-244T00:00:07.134	Stop Time:	2014-244T23:59:58.866
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014245_01

Start Time:	2014-245T00:00:06.835	Stop Time:	2014-245T23:59:57.160
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014246_01

Start Time:	2014-246T00:00:05.129	Stop Time:	2014-246T23:59:54.798
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_2014247_01

Start Time:	2014-247T00:00:02.767	Stop Time:	2014-247T23:59:55.217
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014248_01

Start Time:	2014-248T00:00:03.186	Stop Time:	2014-248T23:59:53.543
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_2014249_01

Start Time:	2014-249T00:00:01.511	Stop Time:	2014-249T23:59:59.899
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_2014250_01

Start Time:	2014-250T00:00:07.868	Stop Time:	2014-250T23:59:59.662
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014251_01

Start Time:	2014-251T00:00:07.631	Stop Time:	2014-251T23:59:56.179
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014252_01

Start Time:	2014-252T00:00:04.144	Stop Time:	2014-252T23:59:52.701
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014253_01

Start Time:	2014-253T00:00:00.775	Stop Time:	2014-253T23:59:55.796
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014254_01

Start Time:	2014-254T00:00:03.764	Stop Time:	2014-254T23:00:37.054
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_2014255_01

Start Time:	2014-255T10:55:24.281	Stop Time:	2014-255T23:59:54.884
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014256_01

Start Time:	2014-256T00:00:02.853	Stop Time:	2014-256T23:59:58.030
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_2014257_01

Start Time:	2014-257T00:00:05.971	Stop Time:	2014-257T23:59:58.410
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014258_01

Start Time:	2014-258T00:00:06.882	Stop Time:	2014-258T23:59:57.091
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_2014259_01

Start Time:	2014-259T00:00:04.333	Stop Time:	2014-259T23:59:55.561
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014260_01

Start Time:	2014-260T00:00:03.529	Stop Time:	2014-260T23:59:54.948
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_2014261_01

Start Time:	2014-261T00:00:02.917	Stop Time:	2014-261T23:59:59.305
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_2014262_01

Start Time:	2014-262T00:00:04.930	Stop Time:	2014-262T23:59:56.880
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_2014263_01

Start Time:	2014-263T00:00:02.505	Stop Time:	2014-263T23:59:55.331
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014264_01

Start Time:	2014-264T00:00:00.956	Stop Time:	2014-264T23:59:54.781
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_2014265_01

Start Time:	2014-265T00:00:00.406	Stop Time:	2014-265T23:59:57.294
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014266_01

Start Time:	2014-266T00:00:05.364	Stop Time:	2014-266T23:59:57.432
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_2014267_01

Start Time:	2014-267T00:00:03.057	Stop Time:	2014-267T23:59:55.566
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014268_01

Start Time:	2014-268T00:00:03.625	Stop Time:	2014-268T23:59:57.434
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_2014269_01

Start Time:	2014-269T00:00:05.376	Stop Time:	2014-269T23:59:53.514
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014270_01

Start Time:	2014-270T00:00:01.447	Stop Time:	2014-270T23:59:56.609
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014271_01

Start Time:	2014-271T00:00:02.234	Stop Time:	2014-271T23:59:53.567
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_2014272_01

Start Time:	2014-272T00:00:01.524	Stop Time:	2014-272T23:59:57.009
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_2014273_01

Start Time:	2014-273T00:00:02.638	Stop Time:	2014-273T23:59:57.460
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_2014274_01

Start Time:	2014-274T00:00:03.089	Stop Time:	2014-274T23:59:59.774
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014275_01

Start Time:	2014-275T00:00:07.809	Stop Time:	2014-275T23:59:55.486
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014276_01

Start Time:	2014-276T00:00:01.111	Stop Time:	2014-276T23:59:53.667
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_2014277_01

Start Time:	2014-277T00:00:01.600	Stop Time:	2014-277T23:59:56.386
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_2014278_01

Start Time:	2014-278T00:00:02.011	Stop Time:	2014-278T23:59:56.837
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014279_01

Start Time:	2014-279T00:00:02.462	Stop Time:	2014-279T23:59:56.287
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_2014280_01

Start Time:	2014-280T00:00:01.912	Stop Time:	2014-280T23:59:56.738
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014281_01

Start Time:	2014-281T00:00:02.363	Stop Time:	2014-281T23:59:57.188
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014282_01

Start Time:	2014-282T00:00:02.813	Stop Time:	2014-282T23:59:56.639
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_2014283_01

Start Time:	2014-283T00:00:02.263	Stop Time:	2014-283T23:59:57.089
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014284_01

Start Time:	2014-284T00:00:02.714	Stop Time:	2014-284T23:59:57.539
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014285_01

Start Time:	2014-285T00:00:03.164	Stop Time:	2014-285T23:59:56.990
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_2014286_01

Start Time:	2014-286T00:00:02.615	Stop Time:	2014-286T23:59:54.440
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014287_01

Start Time:	2014-287T00:00:00.065	Stop Time:	2014-287T19:48:09.862
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_2014288_01

Start Time:	2014-288T11:24:17.133	Stop Time:	2014-288T23:59:56.591
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014289_01

Start Time:	2014-289T00:00:02.216	Stop Time:	2014-289T23:59:57.041
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_2014290_01

Start Time:	2014-290T00:00:02.666	Stop Time:	2014-290T23:59:57.929
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014291_01

Start Time:	2014-291T00:00:04.492	Stop Time:	2014-291T23:59:58.098
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014292_01

Start Time:	2014-292T00:00:06.067	Stop Time:	2014-292T23:59:53.647
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_2014293_01

Start Time:	2014-293T00:00:01.611	Stop Time:	2014-293T23:59:55.023
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014294_01

Start Time:	2014-294T00:00:03.019	Stop Time:	2014-294T23:59:54.200
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014295_01

Start Time:	2014-295T00:00:02.168	Stop Time:	2014-295T06:38:21.766
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014296_01

Start Time:	2014-296T01:31:58.963	Stop Time:	2014-296T23:59:54.694
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_2014297_01

Start Time:	2014-297T00:00:00.319	Stop Time:	2014-297T23:59:54.227
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014298_01

Start Time:	2014-298T00:00:02.274	Stop Time:	2014-298T23:59:55.908
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014299_01

Start Time:	2014-299T00:00:03.876	Stop Time:	2014-299T23:59:55.171
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014300_01

Start Time:	2014-300T00:00:01.733	Stop Time:	2014-300T23:59:58.902
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014301_01

Start Time:	2014-301T00:00:06.871	Stop Time:	2014-301T23:59:52.384
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014302_01

Start Time:	2014-302T00:00:00.353	Stop Time:	2014-302T00:26:02.218
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_2014303_01

Start Time:	2014-303T08:10:10.964	Stop Time:	2014-303T23:59:55.127
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014304_01

Start Time:	2014-304T00:00:03.600	Stop Time:	2014-304T23:59:52.765
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014305_01

Start Time:	2014-305T00:00:00.734	Stop Time:	2014-305T23:59:57.372
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014306_01

Start Time:	2014-306T00:00:05.341	Stop Time:	2014-306T07:00:02.868
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014307_01

Start Time:	2014-307T11:20:11.692	Stop Time:	2014-307T23:59:52.148
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_2014308_01

Start Time:	2014-308T00:00:00.117	Stop Time:	2014-308T23:59:55.567
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_2014309_01

Start Time:	2014-309T00:00:03.536	Stop Time:	2014-309T23:59:53.205
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_2014310_01

Start Time:	2014-310T00:00:01.174	Stop Time:	2014-310T23:59:56.468
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014311_01

Start Time:	2014-311T00:00:04.437	Stop Time:	2014-311T23:59:53.106
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014312_01

Start Time:	2014-312T00:00:01.074	Stop Time:	2014-312T23:59:56.587
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014313_01

Start Time:	2014-313T00:00:04.556	Stop Time:	2014-313T23:59:53.725
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014314_01

Start Time:	2014-314T00:00:01.694	Stop Time:	2014-314T23:59:59.414
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014315_01

Start Time:	2014-315T00:00:07.344	Stop Time:	2014-315T23:59:59.751
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_2014316_01

Start Time:	2014-316T00:00:07.720	Stop Time:	2014-316T23:59:53.971
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014317_01

Start Time:	2014-317T00:00:02.018	Stop Time:	2014-317T23:59:57.777
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014318_01

Start Time:	2014-318T00:00:03.402	Stop Time:	2014-318T23:59:58.227
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014319_01

Start Time:	2014-319T00:00:03.852	Stop Time:	2014-319T23:59:57.678
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014320_01

Start Time:	2014-320T00:00:03.303	Stop Time:	2014-320T23:59:58.128
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_2014321_01

Start Time:	2014-321T00:00:03.753	Stop Time:	2014-321T23:59:56.579
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014322_01

Start Time:	2014-322T00:00:02.204	Stop Time:	2014-322T23:59:58.029
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014323_01

Start Time:	2014-323T00:00:03.654	Stop Time:	2014-323T23:59:57.480
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_2014324_01

Start Time:	2014-324T00:00:03.105	Stop Time:	2014-324T23:59:57.930
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_2014325_01

Start Time:	2014-325T00:00:03.555	Stop Time:	2014-325T23:59:54.509
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014326_01

Start Time:	2014-326T00:00:00.130	Stop Time:	2014-326T23:59:55.081
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014327_01

Start Time:	2014-327T00:00:00.706	Stop Time:	2014-327T23:59:53.410
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014328_01

Start Time:	2014-328T00:00:01.340	Stop Time:	2014-328T23:59:56.607
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014329_01

Start Time:	2014-329T00:00:02.232	Stop Time:	2014-329T23:59:58.057
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014330_01

Start Time:	2014-330T00:00:03.682	Stop Time:	2014-330T23:59:59.633
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_2014331_01

Start Time:	2014-331T00:00:05.257	Stop Time:	2014-331T23:59:54.458
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014332_01

Start Time:	2014-332T00:00:00.083	Stop Time:	2014-332T23:59:54.533
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014333_01

Start Time:	2014-333T00:00:00.158	Stop Time:	2014-333T23:59:54.484
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_2014334_01

Start Time:	2014-334T00:00:00.113	Stop Time:	2014-334T23:59:54.563
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_2014335_01

Start Time:	2014-335T00:00:00.184	Stop Time:	2014-335T23:59:53.939
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014336_01

Start Time:	2014-336T00:00:01.935	Stop Time:	2014-336T23:59:55.464
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_2014337_01

Start Time:	2014-337T00:00:01.085	Stop Time:	2014-337T23:59:57.536
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014338_01

Start Time:	2014-338T00:00:03.161	Stop Time:	2014-338T23:59:53.736
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_2014339_01

Start Time:	2014-339T00:23:59.356	Stop Time:	2014-339T23:59:56.936
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014340_01

Start Time:	2014-340T00:00:02.561	Stop Time:	2014-340T23:59:58.137
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014341_01

Start Time:	2014-341T00:00:03.762	Stop Time:	2014-341T23:59:58.212
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014342_01

Start Time:	2014-342T00:00:03.837	Stop Time:	2014-342T23:59:59.167
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_2014343_01

Start Time:	2014-343T00:00:04.788	Stop Time:	2014-343T23:59:55.863
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014344_01

Start Time:	2014-344T00:00:01.488	Stop Time:	2014-344T23:59:57.251
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014345_01

Start Time:	2014-345T00:00:01.939	Stop Time:	2014-345T23:59:56.764
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_2014346_01

Start Time:	2014-346T00:00:02.389	Stop Time:	2014-346T23:59:56.214
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014347_01

Start Time:	2014-347T00:00:01.839	Stop Time:	2014-347T23:59:56.665
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014348_01

Start Time:	2014-348T00:00:02.290	Stop Time:	2014-348T23:59:58.268
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014349_01

Start Time:	2014-349T00:00:06.131	Stop Time:	2014-349T23:59:57.316
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_2014350_01

Start Time:	2014-350T00:00:02.941	Stop Time:	2014-350T23:59:57.766
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014351_01

Start Time:	2014-351T00:00:03.391	Stop Time:	2014-351T23:59:57.181
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_2014352_01

Start Time:	2014-352T00:00:02.806	Stop Time:	2014-352T23:59:57.630
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014353_01

Start Time:	2014-353T00:00:03.255	Stop Time:	2014-353T23:59:58.080
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014354_01

Start Time:	2014-354T00:00:03.705	Stop Time:	2014-354T23:59:57.529
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_2014355_01

Start Time:	2014-355T00:00:03.154	Stop Time:	2014-355T23:59:57.979
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014356_01

Start Time:	2014-356T00:00:03.604	Stop Time:	2014-356T23:59:58.428
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_2014357_01

Start Time:	2014-357T00:00:04.053	Stop Time:	2014-357T23:59:57.878
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014358_01

Start Time:	2014-358T00:00:03.503	Stop Time:	2014-358T23:59:58.327
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_2014359_01

Start Time:	2014-359T00:00:03.952	Stop Time:	2014-359T23:59:55.535
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014360_01

Start Time:	2014-360T00:00:03.441	Stop Time:	2014-360T23:59:51.953
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014361_01

Start Time:	2014-361T00:00:00.230	Stop Time:	2014-361T23:59:52.301
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_2014362_01

Start Time:	2014-362T00:00:00.269	Stop Time:	2014-362T23:59:57.961
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014363_01

Start Time:	2014-363T00:00:05.879	Stop Time:	2014-363T23:59:57.950
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2014364_01

Start Time:	2014-364T00:00:03.579	Stop Time:	2014-364T23:59:56.899
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_2014365_01

Start Time:	2014-365T00:00:02.524	Stop Time:	2014-365T23:59:54.259
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric 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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