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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/ 2013 /

LACCFULL0_2013001_01

Start Time:	2013-001T00:00:00.559	Stop Time:	2013-001T23:59:56.058
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013002_01

Start Time:	2013-002T00:00:07.073	Stop Time:	2013-002T23:59:52.556
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013003_01

Start Time:	2013-003T00:00:03.325	Stop Time:	2013-003T23:59:56.523
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013004_01

Start Time:	2013-004T00:00:00.273	Stop Time:	2013-004T23:59:56.099
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013005_01

Start Time:	2013-005T00:00:01.724	Stop Time:	2013-005T23:59:56.550
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013006_01

Start Time:	2013-006T00:00:02.175	Stop Time:	2013-006T23:59:56.001
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013007_01

Start Time:	2013-007T00:00:01.626	Stop Time:	2013-007T23:59:58.328
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013008_01

Start Time:	2013-008T00:00:03.953	Stop Time:	2013-008T23:59:57.779
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013009_01

Start Time:	2013-009T00:00:03.404	Stop Time:	2013-009T23:59:59.230
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013010_01

Start Time:	2013-010T00:00:04.855	Stop Time:	2013-010T23:59:58.682
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_2013011_01

Start Time:	2013-011T00:00:04.307	Stop Time:	2013-011T23:59:57.133
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_2013012_01

Start Time:	2013-012T00:00:02.758	Stop Time:	2013-012T23:59:56.584
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_2013013_01

Start Time:	2013-013T00:00:02.209	Stop Time:	2013-013T23:59:57.036
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013014_01

Start Time:	2013-014T00:00:02.660	Stop Time:	2013-014T23:59:57.487
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013015_01

Start Time:	2013-015T00:00:03.112	Stop Time:	2013-015T23:59:50.376
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_2013016_01

Start Time:	2013-016T00:00:01.391	Stop Time:	2013-016T23:59:57.643
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013017_01

Start Time:	2013-017T00:00:08.655	Stop Time:	2013-017T23:59:54.138
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013018_01

Start Time:	2013-018T00:00:05.153	Stop Time:	2013-018T23:59:49.636
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_2013019_01

Start Time:	2013-019T00:00:00.651	Stop Time:	2013-019T23:59:56.368
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013020_01

Start Time:	2013-020T00:00:01.997	Stop Time:	2013-020T23:59:55.819
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013021_01

Start Time:	2013-021T00:00:01.447	Stop Time:	2013-021T23:59:59.270
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013022_01

Start Time:	2013-022T00:00:04.895	Stop Time:	2013-022T23:59:55.846
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013023_01

Start Time:	2013-023T00:00:01.471	Stop Time:	2013-023T23:59:55.297
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013024_01

Start Time:	2013-024T00:00:00.922	Stop Time:	2013-024T23:59:55.749
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013025_01

Start Time:	2013-025T00:00:01.374	Stop Time:	2013-025T23:59:56.200
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_2013026_01

Start Time:	2013-026T00:00:01.825	Stop Time:	2013-026T23:59:55.651
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013027_01

Start Time:	2013-027T00:00:01.276	Stop Time:	2013-027T23:59:59.853
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013028_01

Start Time:	2013-028T00:00:05.477	Stop Time:	2013-028T23:59:54.679
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013029_01

Start Time:	2013-029T00:00:00.304	Stop Time:	2013-029T23:59:58.255
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013030_01

Start Time:	2013-030T00:00:02.005	Stop Time:	2013-030T23:59:57.206
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013031_01

Start Time:	2013-031T00:00:02.831	Stop Time:	2013-031T23:59:57.658
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013032_01

Start Time:	2013-032T00:00:01.408	Stop Time:	2013-032T23:59:57.109
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013033_01

Start Time:	2013-033T00:00:02.734	Stop Time:	2013-033T23:59:54.685
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_2013034_01

Start Time:	2013-034T00:00:00.314	Stop Time:	2013-034T23:59:57.887
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_2013035_01

Start Time:	2013-035T00:00:03.512	Stop Time:	2013-035T23:59:57.338
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013036_01

Start Time:	2013-036T00:00:02.963	Stop Time:	2013-036T23:59:57.789
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013037_01

Start Time:	2013-037T00:00:03.414	Stop Time:	2013-037T23:59:58.240
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_2013038_01

Start Time:	2013-038T00:00:03.865	Stop Time:	2013-038T23:59:57.755
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013039_01

Start Time:	2013-039T00:00:03.380	Stop Time:	2013-039T23:59:58.206
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013040_01

Start Time:	2013-040T00:00:03.831	Stop Time:	2013-040T23:59:58.656
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013041_01

Start Time:	2013-041T00:00:04.281	Stop Time:	2013-041T23:59:58.107
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013042_01

Start Time:	2013-042T00:00:03.732	Stop Time:	2013-042T23:59:58.557
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013043_01

Start Time:	2013-043T00:00:04.182	Stop Time:	2013-043T23:59:54.070
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_2013044_01

Start Time:	2013-044T00:00:05.086	Stop Time:	2013-044T23:59:50.568
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013045_01

Start Time:	2013-045T00:00:01.337	Stop Time:	2013-045T23:59:54.534
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013046_01

Start Time:	2013-046T00:00:00.159	Stop Time:	2013-046T23:59:59.609
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_2013047_01

Start Time:	2013-047T00:00:05.238	Stop Time:	2013-047T23:59:58.185
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_2013048_01

Start Time:	2013-048T00:00:02.872	Stop Time:	2013-048T23:59:56.760
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013049_01

Start Time:	2013-049T00:00:02.385	Stop Time:	2013-049T23:59:57.211
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013050_01

Start Time:	2013-050T00:00:02.836	Stop Time:	2013-050T23:59:54.911
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013051_01

Start Time:	2013-051T00:00:00.536	Stop Time:	2013-051T23:59:55.100
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013052_01

Start Time:	2013-052T00:00:03.147	Stop Time:	2013-052T23:59:56.062
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013053_01

Start Time:	2013-053T00:00:01.687	Stop Time:	2013-053T23:59:56.888
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013054_01

Start Time:	2013-054T00:00:02.513	Stop Time:	2013-054T23:59:58.588
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_2013055_01

Start Time:	2013-055T00:00:02.338	Stop Time:	2013-055T23:59:52.211
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013056_01

Start Time:	2013-056T00:00:00.293	Stop Time:	2013-056T23:59:58.239
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013057_01

Start Time:	2013-057T00:00:01.989	Stop Time:	2013-057T23:59:56.815
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013058_01

Start Time:	2013-058T00:00:02.440	Stop Time:	2013-058T23:59:57.265
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_2013059_01

Start Time:	2013-059T00:00:02.890	Stop Time:	2013-059T23:59:57.716
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013060_01

Start Time:	2013-060T00:00:03.341	Stop Time:	2013-060T23:59:57.166
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_2013061_01

Start Time:	2013-061T00:00:02.791	Stop Time:	2013-061T23:59:57.617
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013062_01

Start Time:	2013-062T00:00:03.242	Stop Time:	2013-062T23:59:58.067
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013063_01

Start Time:	2013-063T00:00:03.692	Stop Time:	2013-063T23:59:57.518
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013064_01

Start Time:	2013-064T00:00:03.143	Stop Time:	2013-064T23:59:57.968
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013065_01

Start Time:	2013-065T00:00:03.593	Stop Time:	2013-065T23:59:57.419
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_2013066_01

Start Time:	2013-066T00:00:03.044	Stop Time:	2013-066T23:59:57.869
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013067_01

Start Time:	2013-067T00:00:03.494	Stop Time:	2013-067T23:59:58.320
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_2013068_01

Start Time:	2013-068T00:00:03.945	Stop Time:	2013-068T23:59:58.769
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_2013069_01

Start Time:	2013-069T00:00:04.394	Stop Time:	2013-069T23:59:59.220
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013070_01

Start Time:	2013-070T00:00:04.845	Stop Time:	2013-070T23:59:58.670
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013071_01

Start Time:	2013-071T00:00:04.295	Stop Time:	2013-071T23:59:59.414
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_2013072_01

Start Time:	2013-072T00:00:07.332	Stop Time:	2013-072T23:59:57.138
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013073_01

Start Time:	2013-073T00:00:04.950	Stop Time:	2013-073T23:59:58.522
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013074_01

Start Time:	2013-074T00:00:04.147	Stop Time:	2013-074T23:59:53.851
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_2013075_01

Start Time:	2013-075T00:00:01.765	Stop Time:	2013-075T23:59:55.013
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013076_01

Start Time:	2013-076T00:00:02.958	Stop Time:	2013-076T23:59:59.655
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_2013077_01

Start Time:	2013-077T00:00:07.623	Stop Time:	2013-077T23:59:57.449
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013078_01

Start Time:	2013-078T00:00:03.074	Stop Time:	2013-078T23:59:57.649
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013079_01

Start Time:	2013-079T00:00:03.274	Stop Time:	2013-079T23:59:59.350
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013080_01

Start Time:	2013-080T00:00:04.975	Stop Time:	2013-080T23:59:55.175
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013081_01

Start Time:	2013-081T00:00:00.800	Stop Time:	2013-081T23:59:58.005
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013082_01

Start Time:	2013-082T00:00:03.626	Stop Time:	2013-082T23:59:58.576
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013083_01

Start Time:	2013-083T00:00:04.201	Stop Time:	2013-083T23:59:57.777
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_2013084_01

Start Time:	2013-084T00:00:03.402	Stop Time:	2013-084T23:59:58.227
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_2013085_01

Start Time:	2013-085T00:00:03.852	Stop Time:	2013-085T23:59:56.803
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013086_01

Start Time:	2013-086T00:00:00.553	Stop Time:	2013-086T23:59:58.253
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013087_01

Start Time:	2013-087T00:00:02.003	Stop Time:	2013-087T23:59:59.954
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013088_01

Start Time:	2013-088T00:00:03.704	Stop Time:	2013-088T23:59:59.904
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013089_01

Start Time:	2013-089T00:00:03.654	Stop Time:	2013-089T23:59:57.605
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013090_01

Start Time:	2013-090T00:00:01.355	Stop Time:	2013-090T23:59:57.305
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_2013091_01

Start Time:	2013-091T00:00:01.055	Stop Time:	2013-091T23:59:58.756
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013092_01

Start Time:	2013-092T00:00:02.506	Stop Time:	2013-092T23:59:59.206
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013093_01

Start Time:	2013-093T00:00:02.956	Stop Time:	2013-093T23:59:55.907
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013094_01

Start Time:	2013-094T00:00:01.532	Stop Time:	2013-094T23:59:56.357
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013095_01

Start Time:	2013-095T00:00:01.982	Stop Time:	2013-095T23:59:56.808
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013096_01

Start Time:	2013-096T00:00:02.433	Stop Time:	2013-096T23:59:56.133
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013097_01

Start Time:	2013-097T00:00:04.075	Stop Time:	2013-097T23:59:53.502
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013098_01

Start Time:	2013-098T00:00:01.521	Stop Time:	2013-098T23:59:58.534
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013099_01

Start Time:	2013-099T00:00:04.159	Stop Time:	2013-099T23:59:58.985
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013100_01

Start Time:	2013-100T00:00:04.610	Stop Time:	2013-100T23:59:57.564
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013101_01

Start Time:	2013-101T00:00:01.310	Stop Time:	2013-101T23:59:58.011
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013102_01

Start Time:	2013-102T00:00:01.761	Stop Time:	2013-102T23:59:58.465
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013103_01

Start Time:	2013-103T00:00:04.086	Stop Time:	2013-103T23:59:58.662
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_2013104_01

Start Time:	2013-104T00:00:04.287	Stop Time:	2013-104T23:59:54.487
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013105_01

Start Time:	2013-105T00:00:00.112	Stop Time:	2013-105T23:59:59.563
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_2013106_01

Start Time:	2013-106T00:00:05.188	Stop Time:	2013-106T23:59:54.388
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013107_01

Start Time:	2013-107T00:00:00.013	Stop Time:	2013-107T23:59:57.718
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013108_01

Start Time:	2013-108T00:00:01.464	Stop Time:	2013-108T23:59:59.168
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013109_01

Start Time:	2013-109T00:00:02.914	Stop Time:	2013-109T23:59:57.740
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013110_01

Start Time:	2013-110T00:00:03.365	Stop Time:	2013-110T23:59:58.190
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013111_01

Start Time:	2013-111T00:00:03.815	Stop Time:	2013-111T23:59:56.766
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_2013112_01

Start Time:	2013-112T00:00:02.391	Stop Time:	2013-112T23:59:57.216
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013113_01

Start Time:	2013-113T00:00:02.841	Stop Time:	2013-113T23:59:57.292
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013114_01

Start Time:	2013-114T00:00:02.917	Stop Time:	2013-114T23:59:57.742
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_2013115_01

Start Time:	2013-115T00:00:03.367	Stop Time:	2013-115T23:59:58.193
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_2013116_01

Start Time:	2013-116T00:00:03.817	Stop Time:	2013-116T23:59:57.643
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013117_01

Start Time:	2013-117T00:00:03.268	Stop Time:	2013-117T23:59:58.468
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_2013118_01

Start Time:	2013-118T00:00:02.222	Stop Time:	2013-118T23:59:59.419
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_2013119_01

Start Time:	2013-119T00:00:03.169	Stop Time:	2013-119T23:59:58.620
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013120_01

Start Time:	2013-120T00:00:02.370	Stop Time:	2013-120T23:59:56.196
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013121_01

Start Time:	2013-121T00:00:01.821	Stop Time:	2013-121T23:59:54.771
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_2013122_01

Start Time:	2013-122T00:00:00.396	Stop Time:	2013-122T23:59:56.542
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013123_01

Start Time:	2013-123T00:00:04.573	Stop Time:	2013-123T23:59:56.422
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013124_01

Start Time:	2013-124T00:00:02.047	Stop Time:	2013-124T23:59:53.377
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013125_01

Start Time:	2013-125T00:00:01.396	Stop Time:	2013-125T23:59:56.573
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013126_01

Start Time:	2013-126T00:00:02.198	Stop Time:	2013-126T23:59:57.024
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013127_01

Start Time:	2013-127T00:00:02.649	Stop Time:	2013-127T23:59:57.474
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013128_01

Start Time:	2013-128T00:00:03.099	Stop Time:	2013-128T23:59:56.925
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_2013129_01

Start Time:	2013-129T00:00:02.550	Stop Time:	2013-129T23:59:57.375
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013130_01

Start Time:	2013-130T00:00:03.000	Stop Time:	2013-130T23:59:57.826
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_2013131_01

Start Time:	2013-131T00:00:03.451	Stop Time:	2013-131T23:59:58.276
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013132_01

Start Time:	2013-132T00:00:03.901	Stop Time:	2013-132T23:59:58.602
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013133_01

Start Time:	2013-133T00:00:04.227	Stop Time:	2013-133T23:59:57.767
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_2013134_01

Start Time:	2013-134T00:00:05.431	Stop Time:	2013-134T23:59:56.303
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013135_01

Start Time:	2013-135T00:00:04.350	Stop Time:	2013-135T23:59:52.754
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_2013136_01

Start Time:	2013-136T00:00:00.801	Stop Time:	2013-136T23:59:57.403
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013137_01

Start Time:	2013-137T00:00:03.028	Stop Time:	2013-137T23:59:58.604
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013138_01

Start Time:	2013-138T00:00:04.229	Stop Time:	2013-138T23:59:59.054
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013139_01

Start Time:	2013-139T00:00:04.679	Stop Time:	2013-139T23:59:57.005
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013140_01

Start Time:	2013-140T00:00:02.630	Stop Time:	2013-140T23:59:56.584
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_2013141_01

Start Time:	2013-141T00:00:02.205	Stop Time:	2013-141T23:59:57.035
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_2013142_01

Start Time:	2013-142T00:00:02.656	Stop Time:	2013-142T23:59:56.485
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_2013143_01

Start Time:	2013-143T00:00:02.106	Stop Time:	2013-143T23:59:58.104
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013144_01

Start Time:	2013-144T00:00:09.119	Stop Time:	2013-144T23:59:58.386
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_2013145_01

Start Time:	2013-145T00:00:06.339	Stop Time:	2013-145T23:59:54.458
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_2013146_01

Start Time:	2013-146T00:00:00.083	Stop Time:	2013-146T23:59:49.486
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_2013147_01

Start Time:	2013-147T00:00:00.502	Stop Time:	2013-147T23:59:55.749
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013148_01

Start Time:	2013-148T00:00:06.765	Stop Time:	2013-148T23:59:59.934
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_2013149_01

Start Time:	2013-149T00:00:05.559	Stop Time:	2013-149T23:59:56.635
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013150_01

Start Time:	2013-150T00:00:00.385	Stop Time:	2013-150T23:59:59.960
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013151_01

Start Time:	2013-151T00:00:05.585	Stop Time:	2013-151T23:59:54.786
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013152_01

Start Time:	2013-152T00:00:00.410	Stop Time:	2013-152T23:59:55.236
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013153_01

Start Time:	2013-153T00:00:00.861	Stop Time:	2013-153T23:59:50.468
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_2013154_01

Start Time:	2013-154T00:00:01.483	Stop Time:	2013-154T23:59:55.512
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013155_01

Start Time:	2013-155T00:00:01.137	Stop Time:	2013-155T23:59:58.337
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013156_01

Start Time:	2013-156T00:00:03.962	Stop Time:	2013-156T23:59:58.413
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013157_01

Start Time:	2013-157T00:00:04.038	Stop Time:	2013-157T23:59:57.926
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013158_01

Start Time:	2013-158T00:00:03.551	Stop Time:	2013-158T23:59:58.377
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013159_01

Start Time:	2013-159T00:00:04.002	Stop Time:	2013-159T23:59:56.328
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013160_01

Start Time:	2013-160T00:00:01.953	Stop Time:	2013-160T23:59:54.780
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013161_01

Start Time:	2013-161T00:00:00.405	Stop Time:	2013-161T23:59:57.606
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013162_01

Start Time:	2013-162T00:00:03.231	Stop Time:	2013-162T23:59:55.561
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_2013163_01

Start Time:	2013-163T00:00:01.182	Stop Time:	2013-163T23:59:59.758
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013164_01

Start Time:	2013-164T00:00:05.383	Stop Time:	2013-164T23:59:59.120
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013165_01

Start Time:	2013-165T00:00:07.061	Stop Time:	2013-165T23:59:57.411
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013166_01

Start Time:	2013-166T00:00:03.036	Stop Time:	2013-166T23:59:58.862
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_2013167_01

Start Time:	2013-167T00:00:04.487	Stop Time:	2013-167T23:59:59.314
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_2013168_01

Start Time:	2013-168T00:00:04.939	Stop Time:	2013-168T23:40:44.648
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013169_01

Start Time:	2013-169T04:28:53.167	Stop Time:	2013-169T23:59:59.217
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_2013170_01

Start Time:	2013-170T00:00:04.842	Stop Time:	2013-170T23:59:59.668
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013171_01

Start Time:	2013-171T00:00:05.293	Stop Time:	2013-171T23:59:59.119
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013172_01

Start Time:	2013-172T00:00:04.744	Stop Time:	2013-172T23:59:59.571
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013173_01

Start Time:	2013-173T00:00:05.196	Stop Time:	2013-173T23:59:56.272
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013174_01

Start Time:	2013-174T00:00:00.022	Stop Time:	2013-174T23:59:56.723
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013175_01

Start Time:	2013-175T00:00:00.473	Stop Time:	2013-175T23:59:55.299
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013176_01

Start Time:	2013-176T00:00:00.924	Stop Time:	2013-176T23:59:59.501
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013177_01

Start Time:	2013-177T00:00:05.126	Stop Time:	2013-177T23:59:59.471
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013178_01

Start Time:	2013-178T00:00:07.331	Stop Time:	2013-178T23:59:53.649
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013179_01

Start Time:	2013-179T00:00:01.634	Stop Time:	2013-179T23:59:55.729
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013180_01

Start Time:	2013-180T00:00:01.354	Stop Time:	2013-180T23:59:56.673
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_2013181_01

Start Time:	2013-181T00:00:04.665	Stop Time:	2013-181T23:59:57.507
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013182_01

Start Time:	2013-182T00:00:03.136	Stop Time:	2013-182T23:59:56.833
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013183_01

Start Time:	2013-183T00:00:02.458	Stop Time:	2013-183T23:59:56.284
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_2013184_01

Start Time:	2013-184T00:00:01.909	Stop Time:	2013-184T23:59:57.958
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013185_01

Start Time:	2013-185T00:00:06.005	Stop Time:	2013-185T23:59:55.812
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013186_01

Start Time:	2013-186T00:00:01.437	Stop Time:	2013-186T23:59:56.392
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_2013187_01

Start Time:	2013-187T00:00:02.013	Stop Time:	2013-187T23:59:57.714
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013188_01

Start Time:	2013-188T00:00:03.339	Stop Time:	2013-188T23:59:59.040
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013189_01

Start Time:	2013-189T00:00:04.665	Stop Time:	2013-189T23:59:59.492
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013190_01

Start Time:	2013-190T00:00:05.117	Stop Time:	2013-190T23:59:59.943
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_2013191_01

Start Time:	2013-191T00:00:05.568	Stop Time:	2013-191T23:59:56.648
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013192_01

Start Time:	2013-192T00:00:02.269	Stop Time:	2013-192T23:59:56.470
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013193_01

Start Time:	2013-193T00:00:02.095	Stop Time:	2013-193T23:59:55.547
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013194_01

Start Time:	2013-194T00:00:01.172	Stop Time:	2013-194T23:59:59.514
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_2013195_01

Start Time:	2013-195T00:00:07.471	Stop Time:	2013-195T23:59:55.934
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_2013196_01

Start Time:	2013-196T00:00:03.992	Stop Time:	2013-196T23:59:58.854
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013197_01

Start Time:	2013-197T00:00:06.850	Stop Time:	2013-197T23:59:53.195
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013198_01

Start Time:	2013-198T00:00:01.164	Stop Time:	2013-198T23:59:54.545
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013199_01

Start Time:	2013-199T00:00:02.529	Stop Time:	2013-199T23:59:56.258
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013200_01

Start Time:	2013-200T00:00:04.250	Stop Time:	2013-200T23:59:57.455
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013201_01

Start Time:	2013-201T00:00:01.205	Stop Time:	2013-201T23:59:59.157
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013202_01

Start Time:	2013-202T00:00:02.907	Stop Time:	2013-202T23:59:59.858
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013203_01

Start Time:	2013-203T00:00:05.483	Stop Time:	2013-203T23:59:57.809
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013204_01

Start Time:	2013-204T00:00:03.434	Stop Time:	2013-204T23:59:54.511
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013205_01

Start Time:	2013-205T00:00:00.136	Stop Time:	2013-205T23:59:54.963
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013206_01

Start Time:	2013-206T00:00:00.588	Stop Time:	2013-206T23:59:59.164
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013207_01

Start Time:	2013-207T00:00:04.789	Stop Time:	2013-207T23:59:59.615
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013208_01

Start Time:	2013-208T00:00:05.240	Stop Time:	2013-208T23:59:57.691
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013209_01

Start Time:	2013-209T00:00:03.320	Stop Time:	2013-209T23:59:54.893
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013210_01

Start Time:	2013-210T00:00:00.518	Stop Time:	2013-210T23:59:54.844
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013211_01

Start Time:	2013-211T00:00:00.469	Stop Time:	2013-211T23:59:54.795
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013212_01

Start Time:	2013-212T00:00:00.420	Stop Time:	2013-212T23:59:56.125
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013213_01

Start Time:	2013-213T00:00:01.746	Stop Time:	2013-213T23:59:55.576
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013214_01

Start Time:	2013-214T00:00:01.198	Stop Time:	2013-214T23:59:54.399
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013215_01

Start Time:	2013-215T00:00:00.028	Stop Time:	2013-215T23:59:54.850
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013216_01

Start Time:	2013-216T00:00:00.479	Stop Time:	2013-216T23:59:55.301
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_2013217_01

Start Time:	2013-217T00:00:00.930	Stop Time:	2013-217T23:59:54.878
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_2013218_01

Start Time:	2013-218T00:00:00.503	Stop Time:	2013-218T23:59:59.079
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013219_01

Start Time:	2013-219T00:00:02.829	Stop Time:	2013-219T23:59:57.780
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013220_01

Start Time:	2013-220T00:00:03.405	Stop Time:	2013-220T23:59:58.735
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013221_01

Start Time:	2013-221T00:00:04.356	Stop Time:	2013-221T23:59:58.186
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013222_01

Start Time:	2013-222T00:00:03.807	Stop Time:	2013-222T23:59:49.649
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013223_01

Start Time:	2013-223T00:00:00.665	Stop Time:	2013-223T23:59:56.163
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013224_01

Start Time:	2013-224T00:00:07.179	Stop Time:	2013-224T23:59:59.693
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013225_01

Start Time:	2013-225T00:00:10.708	Stop Time:	2013-225T23:59:55.191
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013226_01

Start Time:	2013-226T00:00:06.206	Stop Time:	2013-226T23:59:59.939
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_2013227_01

Start Time:	2013-227T00:00:03.689	Stop Time:	2013-227T23:59:58.140
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013228_01

Start Time:	2013-228T00:00:01.894	Stop Time:	2013-228T23:59:57.966
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013229_01

Start Time:	2013-229T00:00:03.591	Stop Time:	2013-229T23:59:57.418
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013230_01

Start Time:	2013-230T00:00:03.042	Stop Time:	2013-230T23:59:57.869
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013231_01

Start Time:	2013-231T00:00:03.494	Stop Time:	2013-231T23:59:57.320
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013232_01

Start Time:	2013-232T00:00:02.945	Stop Time:	2013-232T23:59:57.771
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_2013233_01

Start Time:	2013-233T00:00:03.396	Stop Time:	2013-233T23:59:58.222
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_2013234_01

Start Time:	2013-234T00:00:03.847	Stop Time:	2013-234T23:59:56.799
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013235_01

Start Time:	2013-235T00:00:00.549	Stop Time:	2013-235T23:59:58.250
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013236_01

Start Time:	2013-236T00:00:02.000	Stop Time:	2013-236T23:59:59.701
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_2013237_01

Start Time:	2013-237T00:00:03.451	Stop Time:	2013-237T23:59:57.403
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013238_01

Start Time:	2013-238T00:00:01.152	Stop Time:	2013-238T23:59:58.854
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013239_01

Start Time:	2013-239T00:00:02.604	Stop Time:	2013-239T23:59:57.555
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013240_01

Start Time:	2013-240T00:00:01.305	Stop Time:	2013-240T23:59:59.006
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013241_01

Start Time:	2013-241T00:00:02.756	Stop Time:	2013-241T23:59:59.458
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_2013242_01

Start Time:	2013-242T00:00:05.082	Stop Time:	2013-242T23:59:56.159
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_2013243_01

Start Time:	2013-243T00:00:00.846	Stop Time:	2013-243T23:59:52.981
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013244_01

Start Time:	2013-244T00:00:00.965	Stop Time:	2013-244T23:59:59.061
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013245_01

Start Time:	2013-245T00:00:04.686	Stop Time:	2013-245T23:59:59.263
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013246_01

Start Time:	2013-246T00:00:04.887	Stop Time:	2013-246T23:59:59.714
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013247_01

Start Time:	2013-247T00:00:05.339	Stop Time:	2013-247T23:59:59.915
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013248_01

Start Time:	2013-248T00:00:05.540	Stop Time:	2013-248T23:59:54.741
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013249_01

Start Time:	2013-249T00:00:00.366	Stop Time:	2013-249T23:59:58.821
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013250_01

Start Time:	2013-250T00:00:04.443	Stop Time:	2013-250T23:59:59.269
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013251_01

Start Time:	2013-251T00:00:03.019	Stop Time:	2013-251T23:59:56.970
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013252_01

Start Time:	2013-252T00:00:00.720	Stop Time:	2013-252T23:59:57.422
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013253_01

Start Time:	2013-253T00:00:03.047	Stop Time:	2013-253T23:59:57.624
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013254_01

Start Time:	2013-254T00:00:03.249	Stop Time:	2013-254T23:59:58.075
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013255_01

Start Time:	2013-255T00:00:03.700	Stop Time:	2013-255T23:59:58.014
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013256_01

Start Time:	2013-256T00:00:05.956	Stop Time:	2013-256T23:59:57.477
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_2013257_01

Start Time:	2013-257T00:00:01.227	Stop Time:	2013-257T23:59:58.475
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013258_01

Start Time:	2013-258T00:00:06.483	Stop Time:	2013-258T23:59:59.810
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013259_01

Start Time:	2013-259T00:00:07.790	Stop Time:	2013-259T23:59:58.831
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013260_01

Start Time:	2013-260T00:00:04.456	Stop Time:	2013-260T23:59:58.282
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013261_01

Start Time:	2013-261T00:00:03.907	Stop Time:	2013-261T23:59:58.734
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013262_01

Start Time:	2013-262T00:00:04.359	Stop Time:	2013-262T23:59:56.435
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013263_01

Start Time:	2013-263T00:00:00.185	Stop Time:	2013-263T23:59:57.824
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_2013264_01

Start Time:	2013-264T00:00:02.511	Stop Time:	2013-264T23:59:58.337
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013265_01

Start Time:	2013-265T00:00:02.087	Stop Time:	2013-265T23:59:59.789
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013266_01

Start Time:	2013-266T00:00:04.476	Stop Time:	2013-266T23:59:55.490
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_2013267_01

Start Time:	2013-267T00:00:01.115	Stop Time:	2013-267T23:59:55.941
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_2013268_01

Start Time:	2013-268T00:00:01.566	Stop Time:	2013-268T23:59:56.393
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013269_01

Start Time:	2013-269T00:00:02.017	Stop Time:	2013-269T23:59:55.844
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013270_01

Start Time:	2013-270T00:00:01.469	Stop Time:	2013-270T23:59:58.170
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013271_01

Start Time:	2013-271T00:00:03.795	Stop Time:	2013-271T23:59:58.621
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013272_01

Start Time:	2013-272T00:00:04.246	Stop Time:	2013-272T23:59:55.623
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013273_01

Start Time:	2013-273T00:00:03.580	Stop Time:	2013-273T23:59:59.657
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013274_01

Start Time:	2013-274T00:00:07.664	Stop Time:	2013-274T23:59:56.600
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_2013275_01

Start Time:	2013-275T00:00:00.350	Stop Time:	2013-275T23:59:53.274
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013276_01

Start Time:	2013-276T00:00:01.204	Stop Time:	2013-276T23:59:57.628
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013277_01

Start Time:	2013-277T00:00:03.253	Stop Time:	2013-277T23:59:56.423
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013278_01

Start Time:	2013-278T00:00:04.419	Stop Time:	2013-278T23:59:56.909
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013279_01

Start Time:	2013-279T00:00:02.530	Stop Time:	2013-279T23:59:56.356
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013280_01

Start Time:	2013-280T00:00:01.981	Stop Time:	2013-280T23:59:58.433
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013281_01

Start Time:	2013-281T00:00:04.058	Stop Time:	2013-281T23:59:57.884
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_2013282_01

Start Time:	2013-282T00:00:03.509	Stop Time:	2013-282T23:59:58.335
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013283_01

Start Time:	2013-283T00:00:03.960	Stop Time:	2013-283T23:59:58.787
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_2013284_01

Start Time:	2013-284T00:00:04.411	Stop Time:	2013-284T23:59:58.238
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013285_01

Start Time:	2013-285T00:00:03.863	Stop Time:	2013-285T23:59:58.689
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013286_01

Start Time:	2013-286T00:00:04.314	Stop Time:	2013-286T23:59:57.265
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_2013287_01

Start Time:	2013-287T00:00:01.015	Stop Time:	2013-287T23:59:53.810
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013288_01

Start Time:	2013-288T00:00:01.779	Stop Time:	2013-288T23:59:57.793
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013289_01

Start Time:	2013-289T00:00:03.422	Stop Time:	2013-289T23:59:54.744
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013290_01

Start Time:	2013-290T00:00:00.369	Stop Time:	2013-290T23:59:56.324
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013291_01

Start Time:	2013-291T00:00:01.945	Stop Time:	2013-291T23:59:55.522
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013292_01

Start Time:	2013-292T00:00:01.147	Stop Time:	2013-292T23:59:55.973
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013293_01

Start Time:	2013-293T00:00:01.598	Stop Time:	2013-293T23:59:56.678
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_2013294_01

Start Time:	2013-294T00:00:00.424	Stop Time:	2013-294T23:59:57.129
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013295_01

Start Time:	2013-295T00:00:02.751	Stop Time:	2013-295T23:59:57.581
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013296_01

Start Time:	2013-296T00:00:03.202	Stop Time:	2013-296T23:59:58.032
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_2013297_01

Start Time:	2013-297T00:00:03.653	Stop Time:	2013-297T23:59:57.483
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_2013298_01

Start Time:	2013-298T00:00:03.104	Stop Time:	2013-298T23:59:57.935
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013299_01

Start Time:	2013-299T00:00:03.556	Stop Time:	2013-299T23:59:58.386
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_2013300_01

Start Time:	2013-300T00:00:04.007	Stop Time:	2013-300T23:59:57.837
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013301_01

Start Time:	2013-301T00:00:03.458	Stop Time:	2013-301T23:59:58.288
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013302_01

Start Time:	2013-302T00:00:03.909	Stop Time:	2013-302T23:59:58.740
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013303_01

Start Time:	2013-303T00:00:04.361	Stop Time:	2013-303T23:59:57.311
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013304_01

Start Time:	2013-304T00:00:02.936	Stop Time:	2013-304T23:59:56.762
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013305_01

Start Time:	2013-305T00:00:02.387	Stop Time:	2013-305T23:59:57.214
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_2013306_01

Start Time:	2013-306T00:00:02.839	Stop Time:	2013-306T23:59:57.665
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_2013307_01

Start Time:	2013-307T00:00:03.290	Stop Time:	2013-307T23:59:55.241
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013308_01

Start Time:	2013-308T00:00:00.866	Stop Time:	2013-308T23:59:55.692
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013309_01

Start Time:	2013-309T00:00:01.317	Stop Time:	2013-309T17:49:07.410
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_2013310_01

Start Time:	2013-310T13:25:15.591	Stop Time:	2013-310T23:59:55.595
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013311_01

Start Time:	2013-311T00:00:01.220	Stop Time:	2013-311T23:59:57.046
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013312_01

Start Time:	2013-312T00:00:02.671	Stop Time:	2013-312T23:59:55.498
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013313_01

Start Time:	2013-313T00:00:01.123	Stop Time:	2013-313T11:49:07.352
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013314_01

Start Time:	2013-314T09:01:15.497	Stop Time:	2013-314T23:59:54.400
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013315_01

Start Time:	2013-315T00:00:00.025	Stop Time:	2013-315T23:59:56.851
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_2013316_01

Start Time:	2013-316T00:00:00.601	Stop Time:	2013-316T23:59:57.303
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013317_01

Start Time:	2013-317T00:00:02.928	Stop Time:	2013-317T23:59:57.754
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_2013318_01

Start Time:	2013-318T00:00:03.379	Stop Time:	2013-318T23:59:58.205
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_2013319_01

Start Time:	2013-319T00:00:03.830	Stop Time:	2013-319T23:59:55.782
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_2013320_01

Start Time:	2013-320T00:00:01.407	Stop Time:	2013-320T23:59:56.233
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_2013321_01

Start Time:	2013-321T00:00:01.858	Stop Time:	2013-321T23:59:56.684
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013322_01

Start Time:	2013-322T00:00:02.309	Stop Time:	2013-322T23:59:58.885
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013323_01

Start Time:	2013-323T00:00:04.510	Stop Time:	2013-323T23:59:59.337
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013324_01

Start Time:	2013-324T00:00:04.962	Stop Time:	2013-324T23:59:57.288
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013325_01

Start Time:	2013-325T00:00:02.913	Stop Time:	2013-325T23:59:56.118
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_2013326_01

Start Time:	2013-326T00:00:01.739	Stop Time:	2013-326T23:59:58.941
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_2013327_01

Start Time:	2013-327T00:00:04.570	Stop Time:	2013-327T23:59:56.642
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013328_01

Start Time:	2013-328T00:00:02.267	Stop Time:	2013-328T23:59:56.718
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013329_01

Start Time:	2013-329T00:00:02.343	Stop Time:	2013-329T23:59:56.920
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013330_01

Start Time:	2013-330T00:00:02.544	Stop Time:	2013-330T23:59:58.871
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013331_01

Start Time:	2013-331T00:00:04.496	Stop Time:	2013-331T23:59:57.197
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013332_01

Start Time:	2013-332T00:00:02.826	Stop Time:	2013-332T23:59:59.816
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_2013333_01

Start Time:	2013-333T00:00:07.762	Stop Time:	2013-333T23:59:56.350
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013334_01

Start Time:	2013-334T00:00:01.975	Stop Time:	2013-334T23:59:58.676
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013335_01

Start Time:	2013-335T00:00:01.488	Stop Time:	2013-335T23:59:55.561
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_2013336_01

Start Time:	2013-336T00:00:03.491	Stop Time:	2013-336T23:59:55.204
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013337_01

Start Time:	2013-337T00:00:00.829	Stop Time:	2013-337T23:59:54.534
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013338_01

Start Time:	2013-338T00:00:00.155	Stop Time:	2013-338T23:59:58.606
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013339_01

Start Time:	2013-339T00:00:04.231	Stop Time:	2013-339T23:59:59.682
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_2013340_01

Start Time:	2013-340T00:00:03.432	Stop Time:	2013-340T23:59:56.384
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_2013341_01

Start Time:	2013-341T00:00:00.134	Stop Time:	2013-341T23:59:55.960
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013342_01

Start Time:	2013-342T00:00:01.585	Stop Time:	2013-342T23:59:55.411
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013343_01

Start Time:	2013-343T00:00:01.036	Stop Time:	2013-343T23:59:55.863
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_2013344_01

Start Time:	2013-344T00:00:01.488	Stop Time:	2013-344T23:59:56.314
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_2013345_01

Start Time:	2013-345T00:00:01.939	Stop Time:	2013-345T23:59:55.765
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_2013346_01

Start Time:	2013-346T00:00:01.390	Stop Time:	2013-346T23:59:56.217
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_2013347_01

Start Time:	2013-347T00:00:01.841	Stop Time:	2013-347T23:59:55.668
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013348_01

Start Time:	2013-348T00:00:01.293	Stop Time:	2013-348T23:59:56.119
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013349_01

Start Time:	2013-349T00:00:01.744	Stop Time:	2013-349T23:59:56.570
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013350_01

Start Time:	2013-350T00:00:02.195	Stop Time:	2013-350T23:59:56.022
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013351_01

Start Time:	2013-351T00:00:01.647	Stop Time:	2013-351T23:59:54.597
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013352_01

Start Time:	2013-352T00:00:00.222	Stop Time:	2013-352T23:59:54.662
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_2013353_01

Start Time:	2013-353T00:00:02.775	Stop Time:	2013-353T23:59:55.754
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_2013354_01

Start Time:	2013-354T00:00:01.375	Stop Time:	2013-354T23:59:59.576
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013355_01

Start Time:	2013-355T00:00:05.205	Stop Time:	2013-355T23:59:54.402
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013356_01

Start Time:	2013-356T00:00:00.027	Stop Time:	2013-356T23:59:54.854
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013357_01

Start Time:	2013-357T00:00:00.478	Stop Time:	2013-357T23:59:59.930
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_2013358_01

Start Time:	2013-358T00:00:05.559	Stop Time:	2013-358T23:59:54.756
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013359_01

Start Time:	2013-359T00:00:00.381	Stop Time:	2013-359T23:59:55.207
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013360_01

Start Time:	2013-360T00:00:00.832	Stop Time:	2013-360T23:59:54.659
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013361_01

Start Time:	2013-361T00:00:00.284	Stop Time:	2013-361T23:59:55.032
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_2013362_01

Start Time:	2013-362T00:00:00.657	Stop Time:	2013-362T23:59:56.315
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013363_01

Start Time:	2013-363T00:00:04.245	Stop Time:	2013-363T23:59:55.934
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_2013364_01

Start Time:	2013-364T00:00:01.559	Stop Time:	2013-364T23:59:52.459
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

LACCFULL0_2013365_01

Start Time:	2013-365T00:00:00.416	Stop Time:	2013-365T23:59:54.586
The data columns contain full time resolution of LEMMS accumulator rates data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file ( described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). The channels A0 through A8 are measured by the low energy end of LEMMS (the Low Energy Telescope, or LET), and for protons these channels have an energy range of 27 to 4000 keV. The P1 through P9 channels capture protons as measured by the LEMMS High Energy Telescope (HET) and have an energy range of 1 to 60 MeV. Channels C0 through C7 measure electrons, and have an energy of 20 to 900 keV. The E0 through E4 channels are also electrons covering the 150 to 3000 keV range. Also included are the active priority channels respective to the datas time interval, and The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET and HET.

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