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Cassini >> MIMI

CASSINI SATURN MIMI LEMMS CALIBRATED DATA ARCHIVE
CO-S-MIMI-4-LEMMS-CALIB-V1.0	PDS 3 CERTIFIED

Start Time: 2004-01-01 08:00:00 - Stop Time: 2017-09-16 10:00:00

CASSINI SATURN MIMI LEMMS CALIBRATED DATA ARCHIVE

Citiation Information

Author	Vandegriff J., Kusterer M.B.
Title	CASSINI SATURN MIMI LEMMS CALIBRATED DATA ARCHIVE
Publisher	NASA Planetary Data System
Publication Year	2018
doi	https://doi.org/10.17189/1519608

Top/ DATA/ LPHAFULL0/ 2005 /

LPHAFULL0_2005001_01

Start Time:	2005-001T00:00:02.323	Stop Time:	2005-001T23:59:48.761
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005002_01

Start Time:	2005-002T00:00:03.761	Stop Time:	2005-002T23:59:57.698
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005003_01

Start Time:	2005-003T00:00:01.448	Stop Time:	2005-003T23:59:59.136
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005004_01

Start Time:	2005-004T00:00:02.886	Stop Time:	2005-004T23:59:57.823
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005005_01

Start Time:	2005-005T00:00:01.573	Stop Time:	2005-005T23:59:59.261
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005006_01

Start Time:	2005-006T00:00:03.011	Stop Time:	2005-006T11:42:37.486
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005015_01

Start Time:	2005-015T16:49:30.058	Stop Time:	2005-015T23:59:59.886
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005016_01

Start Time:	2005-016T00:00:14.885	Stop Time:	2005-016T23:59:49.323
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005017_01

Start Time:	2005-017T00:00:04.323	Stop Time:	2005-017T23:59:58.260
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005018_01

Start Time:	2005-018T00:00:02.010	Stop Time:	2005-018T23:59:57.198
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005019_01

Start Time:	2005-019T00:00:00.948	Stop Time:	2005-019T23:59:57.135
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005020_01

Start Time:	2005-020T00:00:00.885	Stop Time:	2005-020T23:59:57.072
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005021_01

Start Time:	2005-021T00:00:00.822	Stop Time:	2005-021T23:59:59.509
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005022_01

Start Time:	2005-022T00:00:03.259	Stop Time:	2005-022T23:59:55.279
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005023_01

Start Time:	2005-023T00:00:01.591	Stop Time:	2005-023T23:59:59.884
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005024_01

Start Time:	2005-024T00:00:03.634	Stop Time:	2005-024T23:59:59.322
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005025_01

Start Time:	2005-025T00:00:03.072	Stop Time:	2005-025T23:59:57.009
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005026_01

Start Time:	2005-026T00:00:00.759	Stop Time:	2005-026T23:59:57.697
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005027_01

Start Time:	2005-027T00:00:01.447	Stop Time:	2005-027T23:59:58.884
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005028_01

Start Time:	2005-028T00:00:02.634	Stop Time:	2005-028T23:59:54.943
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005029_01

Start Time:	2005-029T00:00:06.126	Stop Time:	2005-029T23:59:54.529
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005030_01

Start Time:	2005-030T00:00:01.013	Stop Time:	2005-030T23:59:59.220
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005031_01

Start Time:	2005-031T00:00:05.497	Stop Time:	2005-031T23:59:59.134
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005032_01

Start Time:	2005-032T00:00:03.888	Stop Time:	2005-032T23:59:56.325
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005033_01

Start Time:	2005-033T00:00:02.599	Stop Time:	2005-033T23:59:56.388
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005034_01

Start Time:	2005-034T00:00:02.763	Stop Time:	2005-034T23:59:56.697
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005035_01

Start Time:	2005-035T00:00:04.196	Stop Time:	2005-035T23:59:56.388
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005036_01

Start Time:	2005-036T00:00:02.735	Stop Time:	2005-036T23:59:57.571
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005037_01

Start Time:	2005-037T00:00:01.321	Stop Time:	2005-037T23:59:50.599
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005038_01

Start Time:	2005-038T00:00:03.122	Stop Time:	2005-038T23:59:57.946
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005039_01

Start Time:	2005-039T00:00:05.446	Stop Time:	2005-039T23:59:57.634
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005040_01

Start Time:	2005-040T00:00:01.384	Stop Time:	2005-040T23:59:59.825
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005041_01

Start Time:	2005-041T00:00:03.571	Stop Time:	2005-041T23:59:54.767
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005042_01

Start Time:	2005-042T00:00:01.067	Stop Time:	2005-042T23:59:59.196
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005043_01

Start Time:	2005-043T00:00:06.696	Stop Time:	2005-043T23:59:56.188
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005044_01

Start Time:	2005-044T00:00:02.481	Stop Time:	2005-044T23:59:59.071
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005045_01

Start Time:	2005-045T00:00:02.821	Stop Time:	2005-045T23:59:57.013
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005046_01

Start Time:	2005-046T00:00:00.759	Stop Time:	2005-046T23:59:59.450
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005047_01

Start Time:	2005-047T00:00:03.196	Stop Time:	2005-047T23:59:57.071
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005048_01

Start Time:	2005-048T00:00:00.884	Stop Time:	2005-048T23:59:46.321
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005049_01

Start Time:	2005-049T00:00:08.821	Stop Time:	2005-049T23:59:46.759
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005050_01

Start Time:	2005-050T00:00:09.258	Stop Time:	2005-050T23:59:47.196
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005051_01

Start Time:	2005-051T00:00:09.696	Stop Time:	2005-051T23:59:43.634
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005052_01

Start Time:	2005-052T00:00:06.133	Stop Time:	2005-052T23:59:49.075
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005053_01

Start Time:	2005-053T00:00:00.321	Stop Time:	2005-053T23:59:59.758
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005054_01

Start Time:	2005-054T00:00:11.008	Stop Time:	2005-054T23:59:48.415
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005055_01

Start Time:	2005-055T00:00:01.149	Stop Time:	2005-055T23:59:50.059
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005056_01

Start Time:	2005-056T00:00:03.387	Stop Time:	2005-056T23:59:59.243
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005057_01

Start Time:	2005-057T00:00:11.813	Stop Time:	2005-057T23:59:58.778
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005058_01

Start Time:	2005-058T00:00:02.528	Stop Time:	2005-058T23:59:49.360
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005059_01

Start Time:	2005-059T00:00:01.993	Stop Time:	2005-059T23:59:57.772
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005060_01

Start Time:	2005-060T00:00:09.022	Stop Time:	2005-060T23:59:51.978
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005061_01

Start Time:	2005-061T00:00:03.228	Stop Time:	2005-061T23:59:47.402
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005062_01

Start Time:	2005-062T00:00:00.187	Stop Time:	2005-062T23:59:51.562
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005063_01

Start Time:	2005-063T00:00:02.808	Stop Time:	2005-063T23:08:28.523
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005064_01

Start Time:	2005-064T04:04:55.912	Stop Time:	2005-064T23:59:59.451
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005065_01

Start Time:	2005-065T00:00:12.037	Stop Time:	2005-065T23:59:49.001
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005066_01

Start Time:	2005-066T00:00:01.556	Stop Time:	2005-066T23:59:59.086
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005067_01

Start Time:	2005-067T00:00:10.336	Stop Time:	2005-067T23:59:49.781
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005068_01

Start Time:	2005-068T00:00:04.781	Stop Time:	2005-068T23:59:51.228
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005069_01

Start Time:	2005-069T00:00:02.474	Stop Time:	2005-069T23:59:59.169
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005070_01

Start Time:	2005-070T00:00:02.919	Stop Time:	2005-070T23:59:56.863
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005071_01

Start Time:	2005-071T00:00:00.613	Stop Time:	2005-071T23:59:59.808
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005072_01

Start Time:	2005-072T00:00:11.057	Stop Time:	2005-072T23:59:49.002
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005073_01

Start Time:	2005-073T00:00:00.252	Stop Time:	2005-073T23:59:49.446
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005074_01

Start Time:	2005-074T00:00:00.696	Stop Time:	2005-074T23:59:15.633
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005075_01

Start Time:	2005-075T00:00:00.371	Stop Time:	2005-075T23:59:35.683
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005076_01

Start Time:	2005-076T00:00:00.855	Stop Time:	2005-076T23:59:58.784
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005077_01

Start Time:	2005-077T00:00:23.889	Stop Time:	2005-077T23:59:36.228
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005078_01

Start Time:	2005-078T00:00:01.400	Stop Time:	2005-078T23:59:55.169
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005079_01

Start Time:	2005-079T00:00:02.669	Stop Time:	2005-079T23:59:56.613
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005080_01

Start Time:	2005-080T00:00:04.113	Stop Time:	2005-080T23:59:59.175
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005081_01

Start Time:	2005-081T00:00:11.776	Stop Time:	2005-081T23:59:54.592
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005082_01

Start Time:	2005-082T00:00:07.178	Stop Time:	2005-082T23:59:48.158
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005083_01

Start Time:	2005-083T00:00:00.728	Stop Time:	2005-083T23:59:59.450
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005084_01

Start Time:	2005-084T00:00:12.895	Stop Time:	2005-084T23:59:52.746
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005085_01

Start Time:	2005-085T00:00:05.351	Stop Time:	2005-085T23:59:51.553
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005086_01

Start Time:	2005-086T00:00:04.108	Stop Time:	2005-086T23:59:53.322
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005087_01

Start Time:	2005-087T00:00:05.939	Stop Time:	2005-087T23:59:56.169
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005088_01

Start Time:	2005-088T00:00:07.419	Stop Time:	2005-088T23:59:56.613
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005089_01

Start Time:	2005-089T00:00:00.363	Stop Time:	2005-089T23:59:58.058
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005090_01

Start Time:	2005-090T00:00:09.308	Stop Time:	2005-090T23:59:58.502
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005091_01

Start Time:	2005-091T00:00:02.252	Stop Time:	2005-091T23:59:59.947
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005092_01

Start Time:	2005-092T00:00:03.696	Stop Time:	2005-092T23:59:47.700
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005093_01

Start Time:	2005-093T00:00:00.301	Stop Time:	2005-093T23:59:59.835
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005094_01

Start Time:	2005-094T00:00:07.335	Stop Time:	2005-094T23:59:58.780
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005095_01

Start Time:	2005-095T00:00:06.280	Stop Time:	2005-095T00:13:06.275
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005096_01

Start Time:	2005-096T00:29:09.217	Stop Time:	2005-096T23:59:57.430
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005097_01

Start Time:	2005-097T00:00:10.016	Stop Time:	2005-097T23:59:56.203
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005098_01

Start Time:	2005-098T00:00:21.250	Stop Time:	2005-098T23:59:47.558
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005099_01

Start Time:	2005-099T00:00:02.562	Stop Time:	2005-099T23:59:56.502
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005100_01

Start Time:	2005-100T00:00:04.006	Stop Time:	2005-100T23:59:48.228
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005101_01

Start Time:	2005-101T00:00:00.845	Stop Time:	2005-101T23:59:51.963
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005102_01

Start Time:	2005-102T00:00:04.498	Stop Time:	2005-102T23:59:43.769
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005103_01

Start Time:	2005-103T00:00:00.132	Stop Time:	2005-103T23:59:49.184
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005104_01

Start Time:	2005-104T00:00:01.856	Stop Time:	2005-104T23:59:38.798
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005105_01

Start Time:	2005-105T00:00:01.298	Stop Time:	2005-105T23:59:56.744
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005106_01

Start Time:	2005-106T00:00:04.244	Stop Time:	2005-106T23:59:56.691
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005107_01

Start Time:	2005-107T00:00:04.191	Stop Time:	2005-107T23:59:58.641
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005108_01

Start Time:	2005-108T00:00:09.887	Stop Time:	2005-108T23:59:52.380
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005109_01

Start Time:	2005-109T00:00:04.837	Stop Time:	2005-109T23:59:55.529
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005110_01

Start Time:	2005-110T00:00:06.779	Stop Time:	2005-110T23:59:56.226
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005111_01

Start Time:	2005-111T00:00:07.476	Stop Time:	2005-111T23:59:59.172
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005112_01

Start Time:	2005-112T00:00:02.922	Stop Time:	2005-112T23:59:57.118
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005113_01

Start Time:	2005-113T00:00:00.872	Stop Time:	2005-113T23:59:58.564
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005114_01

Start Time:	2005-114T00:00:09.814	Stop Time:	2005-114T23:59:58.765
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005115_01

Start Time:	2005-115T00:00:11.432	Stop Time:	2005-115T23:59:44.625
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005116_01

Start Time:	2005-116T00:00:01.043	Stop Time:	2005-116T23:59:49.927
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005117_01

Start Time:	2005-117T00:00:02.559	Stop Time:	2005-117T23:59:54.381
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005118_01

Start Time:	2005-118T00:00:06.951	Stop Time:	2005-118T23:59:56.069
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005119_01

Start Time:	2005-119T00:00:09.593	Stop Time:	2005-119T23:59:49.243
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005120_01

Start Time:	2005-120T00:00:00.493	Stop Time:	2005-120T23:59:49.689
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005121_01

Start Time:	2005-121T00:00:00.939	Stop Time:	2005-121T23:59:50.386
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005122_01

Start Time:	2005-122T00:00:01.635	Stop Time:	2005-122T23:59:51.082
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005123_01

Start Time:	2005-123T00:00:02.332	Stop Time:	2005-123T23:59:56.278
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005124_01

Start Time:	2005-124T00:00:00.028	Stop Time:	2005-124T23:59:59.974
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005125_01

Start Time:	2005-125T00:00:03.724	Stop Time:	2005-125T23:59:55.362
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005126_01

Start Time:	2005-126T00:00:01.631	Stop Time:	2005-126T23:59:56.121
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005127_01

Start Time:	2005-127T00:00:07.367	Stop Time:	2005-127T23:59:47.633
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005128_01

Start Time:	2005-128T00:00:02.641	Stop Time:	2005-128T23:59:53.013
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005129_01

Start Time:	2005-129T00:00:05.630	Stop Time:	2005-129T23:59:52.686
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005130_01

Start Time:	2005-130T00:00:05.225	Stop Time:	2005-130T23:59:59.906
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005131_01

Start Time:	2005-131T00:00:11.152	Stop Time:	2005-131T23:59:54.723
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005132_01

Start Time:	2005-132T00:00:00.352	Stop Time:	2005-132T23:59:49.544
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005133_01

Start Time:	2005-133T00:00:00.798	Stop Time:	2005-133T23:59:49.991
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005134_01

Start Time:	2005-134T00:00:01.244	Stop Time:	2005-134T23:59:57.765
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005135_01

Start Time:	2005-135T00:00:10.304	Stop Time:	2005-135T23:59:59.633
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005136_01

Start Time:	2005-136T00:00:03.383	Stop Time:	2005-136T23:59:56.896
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005137_01

Start Time:	2005-137T00:00:03.196	Stop Time:	2005-137T23:59:56.276
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005138_01

Start Time:	2005-138T00:00:00.025	Stop Time:	2005-138T23:59:57.843
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005139_01

Start Time:	2005-139T00:00:20.214	Stop Time:	2005-139T23:59:53.668
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005140_01

Start Time:	2005-140T00:00:04.922	Stop Time:	2005-140T23:59:54.114
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005141_01

Start Time:	2005-141T00:00:05.368	Stop Time:	2005-141T23:59:50.811
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005142_01

Start Time:	2005-142T00:00:02.060	Stop Time:	2005-142T23:59:51.257
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005143_01

Start Time:	2005-143T00:00:13.757	Stop Time:	2005-143T23:59:39.941
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005144_01

Start Time:	2005-144T00:00:05.179	Stop Time:	2005-144T23:59:51.649
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005145_01

Start Time:	2005-145T00:00:02.899	Stop Time:	2005-145T23:59:56.845
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005146_01

Start Time:	2005-146T00:00:00.599	Stop Time:	2005-146T23:59:58.292
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005147_01

Start Time:	2005-147T00:00:02.046	Stop Time:	2005-147T23:59:58.988
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005148_01

Start Time:	2005-148T00:00:02.738	Stop Time:	2005-148T23:59:59.434
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005149_01

Start Time:	2005-149T00:00:10.684	Stop Time:	2005-149T23:59:56.619
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005150_01

Start Time:	2005-150T00:00:09.240	Stop Time:	2005-150T23:59:56.174
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005151_01

Start Time:	2005-151T00:00:08.760	Stop Time:	2005-151T23:59:50.778
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005152_01

Start Time:	2005-152T00:00:03.337	Stop Time:	2005-152T23:59:49.204
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005153_01

Start Time:	2005-153T00:00:01.774	Stop Time:	2005-153T23:59:54.837
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005154_01

Start Time:	2005-154T00:00:07.438	Stop Time:	2005-154T23:59:55.091
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005155_01

Start Time:	2005-155T00:00:07.696	Stop Time:	2005-155T23:59:52.380
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005156_01

Start Time:	2005-156T00:00:03.630	Stop Time:	2005-156T23:59:52.829
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005157_01

Start Time:	2005-157T00:00:04.079	Stop Time:	2005-157T23:59:52.938
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005158_01

Start Time:	2005-158T00:00:05.587	Stop Time:	2005-158T23:59:52.978
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005159_01

Start Time:	2005-159T00:00:04.227	Stop Time:	2005-159T23:59:49.677
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005160_01

Start Time:	2005-160T00:00:00.927	Stop Time:	2005-160T23:59:55.376
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005161_01

Start Time:	2005-161T00:00:06.626	Stop Time:	2005-161T23:59:53.075
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005162_01

Start Time:	2005-162T00:00:04.325	Stop Time:	2005-162T23:59:57.775
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005163_01

Start Time:	2005-163T00:00:01.525	Stop Time:	2005-163T23:59:59.962
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005164_01

Start Time:	2005-164T00:00:06.275	Stop Time:	2005-164T23:59:49.173
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005165_01

Start Time:	2005-165T00:00:00.423	Stop Time:	2005-165T23:59:53.626
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005166_01

Start Time:	2005-166T00:00:06.341	Stop Time:	2005-166T23:59:54.572
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005167_01

Start Time:	2005-167T00:00:05.822	Stop Time:	2005-167T23:59:48.092
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005168_01

Start Time:	2005-168T00:00:00.663	Stop Time:	2005-168T23:59:54.721
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005169_01

Start Time:	2005-169T00:00:05.975	Stop Time:	2005-169T23:59:59.424
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005170_01

Start Time:	2005-170T00:00:10.670	Stop Time:	2005-170T23:59:55.874
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005171_01

Start Time:	2005-171T00:00:07.120	Stop Time:	2005-171T23:59:55.878
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005172_01

Start Time:	2005-172T00:00:08.323	Stop Time:	2005-172T23:59:52.018
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005173_01

Start Time:	2005-173T00:00:03.268	Stop Time:	2005-173T23:59:56.030
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005174_01

Start Time:	2005-174T00:00:08.663	Stop Time:	2005-174T23:59:51.917
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005175_01

Start Time:	2005-175T00:00:03.167	Stop Time:	2005-175T23:59:58.866
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005176_01

Start Time:	2005-176T00:00:02.616	Stop Time:	2005-176T23:59:58.522
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005177_01

Start Time:	2005-177T00:00:04.847	Stop Time:	2005-177T23:59:53.019
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005178_01

Start Time:	2005-178T00:00:04.265	Stop Time:	2005-178T23:59:52.468
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005179_01

Start Time:	2005-179T00:00:03.714	Stop Time:	2005-179T23:59:55.194
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005180_01

Start Time:	2005-180T00:00:01.480	Stop Time:	2005-180T23:59:55.245
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005181_01

Start Time:	2005-181T00:00:08.366	Stop Time:	2005-181T23:59:51.030
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005182_01

Start Time:	2005-182T00:00:02.816	Stop Time:	2005-182T23:59:48.003
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005183_01

Start Time:	2005-183T00:00:10.370	Stop Time:	2005-183T23:59:54.710
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005184_01

Start Time:	2005-184T00:00:02.210	Stop Time:	2005-184T23:59:55.160
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005185_01

Start Time:	2005-185T00:00:02.659	Stop Time:	2005-185T23:59:51.359
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005186_01

Start Time:	2005-186T00:00:02.613	Stop Time:	2005-186T23:59:43.277
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005187_01

Start Time:	2005-187T00:00:05.644	Stop Time:	2005-187T23:59:52.929
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005188_01

Start Time:	2005-188T00:00:05.499	Stop Time:	2005-188T23:59:58.207
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005189_01

Start Time:	2005-189T00:00:09.456	Stop Time:	2005-189T23:59:52.156
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005190_01

Start Time:	2005-190T00:00:03.406	Stop Time:	2005-190T23:59:48.855
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005191_01

Start Time:	2005-191T00:00:00.105	Stop Time:	2005-191T23:59:59.054
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005192_01

Start Time:	2005-192T00:00:10.308	Stop Time:	2005-192T23:59:54.461
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005193_01

Start Time:	2005-193T00:00:05.711	Stop Time:	2005-193T23:59:54.658
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005194_01

Start Time:	2005-194T00:00:00.283	Stop Time:	2005-194T23:59:57.050
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005195_01

Start Time:	2005-195T00:00:09.608	Stop Time:	2005-195T23:59:55.301
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005196_01

Start Time:	2005-196T00:00:06.551	Stop Time:	2005-196T23:59:40.998
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005197_01

Start Time:	2005-197T00:00:03.498	Stop Time:	2005-197T23:59:52.695
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005198_01

Start Time:	2005-198T00:00:03.945	Stop Time:	2005-198T23:59:51.891
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005199_01

Start Time:	2005-199T00:00:03.141	Stop Time:	2005-199T23:59:59.088
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005200_01

Start Time:	2005-200T00:00:10.338	Stop Time:	2005-200T18:41:36.157
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005201_01

Start Time:	2005-201T00:23:27.279	Stop Time:	2005-201T23:59:54.981
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005202_01

Start Time:	2005-202T00:00:06.231	Stop Time:	2005-202T23:59:54.428
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005203_01

Start Time:	2005-203T00:00:05.678	Stop Time:	2005-203T23:59:53.875
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005204_01

Start Time:	2005-204T00:00:05.124	Stop Time:	2005-204T23:59:54.322
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005205_01

Start Time:	2005-205T00:00:05.572	Stop Time:	2005-205T23:59:54.769
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005206_01

Start Time:	2005-206T00:00:06.019	Stop Time:	2005-206T23:59:55.216
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005207_01

Start Time:	2005-207T00:00:06.465	Stop Time:	2005-207T23:59:51.912
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005208_01

Start Time:	2005-208T00:00:03.162	Stop Time:	2005-208T23:59:55.109
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005209_01

Start Time:	2005-209T00:00:06.359	Stop Time:	2005-209T23:59:55.805
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005210_01

Start Time:	2005-210T00:00:07.055	Stop Time:	2005-210T23:59:58.252
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005211_01

Start Time:	2005-211T00:00:09.502	Stop Time:	2005-211T23:59:58.699
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005212_01

Start Time:	2005-212T00:00:09.949	Stop Time:	2005-212T23:59:59.145
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005213_01

Start Time:	2005-213T00:00:10.395	Stop Time:	2005-213T23:59:58.842
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005214_01

Start Time:	2005-214T00:00:10.096	Stop Time:	2005-214T23:59:53.539
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005215_01

Start Time:	2005-215T00:00:04.789	Stop Time:	2005-215T23:59:53.985
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005216_01

Start Time:	2005-216T00:00:05.235	Stop Time:	2005-216T23:59:54.432
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005217_01

Start Time:	2005-217T00:00:05.682	Stop Time:	2005-217T23:59:49.129
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005218_01

Start Time:	2005-218T00:00:00.379	Stop Time:	2005-218T23:59:57.825
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005219_01

Start Time:	2005-219T00:00:05.325	Stop Time:	2005-219T23:59:55.776
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005220_01

Start Time:	2005-220T00:00:03.272	Stop Time:	2005-220T23:59:53.223
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005221_01

Start Time:	2005-221T00:00:00.719	Stop Time:	2005-221T23:59:48.915
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005222_01

Start Time:	2005-222T00:00:00.165	Stop Time:	2005-222T23:59:49.362
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005223_01

Start Time:	2005-223T00:00:00.612	Stop Time:	2005-223T23:59:49.809
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005224_01

Start Time:	2005-224T00:00:01.059	Stop Time:	2005-224T23:59:55.255
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005225_01

Start Time:	2005-225T00:00:06.505	Stop Time:	2005-225T23:59:53.702
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005226_01

Start Time:	2005-226T00:00:04.952	Stop Time:	2005-226T23:59:49.149
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005227_01

Start Time:	2005-227T00:00:00.399	Stop Time:	2005-227T23:59:42.845
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005228_01

Start Time:	2005-228T00:00:05.345	Stop Time:	2005-228T23:59:58.292
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005229_01

Start Time:	2005-229T00:00:05.792	Stop Time:	2005-229T23:59:57.243
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005230_01

Start Time:	2005-230T00:00:00.989	Stop Time:	2005-230T23:59:57.435
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005231_01

Start Time:	2005-231T00:00:01.185	Stop Time:	2005-231T23:59:59.632
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005232_01

Start Time:	2005-232T00:00:03.382	Stop Time:	2005-232T23:59:53.583
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005233_01

Start Time:	2005-233T00:00:04.829	Stop Time:	2005-233T23:59:56.775
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005234_01

Start Time:	2005-234T00:00:00.525	Stop Time:	2005-234T23:59:58.222
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005235_01

Start Time:	2005-235T00:00:01.972	Stop Time:	2005-235T23:59:59.669
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005236_01

Start Time:	2005-236T00:00:10.922	Stop Time:	2005-236T23:59:51.615
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005237_01

Start Time:	2005-237T00:00:02.865	Stop Time:	2005-237T23:59:50.812
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005238_01

Start Time:	2005-238T00:00:02.062	Stop Time:	2005-238T23:59:51.259
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005239_01

Start Time:	2005-239T00:00:02.509	Stop Time:	2005-239T23:59:57.205
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005240_01

Start Time:	2005-240T00:00:08.455	Stop Time:	2005-240T23:59:59.902
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005241_01

Start Time:	2005-241T00:00:11.156	Stop Time:	2005-241T23:59:55.599
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005242_01

Start Time:	2005-242T00:00:03.099	Stop Time:	2005-242T23:59:57.049
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005243_01

Start Time:	2005-243T00:00:00.795	Stop Time:	2005-243T23:59:58.496
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005244_01

Start Time:	2005-244T00:00:09.742	Stop Time:	2005-244T17:55:16.829
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005245_01

Start Time:	2005-245T03:31:29.861	Stop Time:	2005-245T23:59:58.135
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005246_01

Start Time:	2005-246T00:00:01.885	Stop Time:	2005-246T23:59:56.832
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005247_01

Start Time:	2005-247T00:00:00.582	Stop Time:	2005-247T23:59:59.529
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005248_01

Start Time:	2005-248T00:00:03.279	Stop Time:	2005-248T23:46:14.981
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005249_01

Start Time:	2005-249T10:57:24.477	Stop Time:	2005-249T23:59:58.422
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005250_01

Start Time:	2005-250T00:00:09.672	Stop Time:	2005-250T08:25:55.353
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005251_01

Start Time:	2005-251T02:50:02.557	Stop Time:	2005-251T23:59:54.069
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005252_01

Start Time:	2005-252T00:00:05.315	Stop Time:	2005-252T23:59:52.763
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005253_01

Start Time:	2005-253T00:00:04.013	Stop Time:	2005-253T23:59:52.210
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005254_01

Start Time:	2005-254T00:00:03.460	Stop Time:	2005-254T23:59:52.719
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005255_01

Start Time:	2005-255T00:00:03.968	Stop Time:	2005-255T23:59:55.666
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005256_01

Start Time:	2005-256T00:00:06.916	Stop Time:	2005-256T23:59:56.364
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005257_01

Start Time:	2005-257T00:00:07.614	Stop Time:	2005-257T23:59:50.816
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005258_01

Start Time:	2005-258T00:00:02.062	Stop Time:	2005-258T23:59:58.510
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005259_01

Start Time:	2005-259T00:00:09.760	Stop Time:	2005-259T23:59:50.208
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005260_01

Start Time:	2005-260T00:00:01.458	Stop Time:	2005-260T23:59:58.656
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005261_01

Start Time:	2005-261T00:00:09.906	Stop Time:	2005-261T23:59:59.104
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005262_01

Start Time:	2005-262T00:00:10.354	Stop Time:	2005-262T17:32:24.951
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005263_01

Start Time:	2005-263T03:08:37.984	Stop Time:	2005-264T00:00:00.000
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005264_01

Start Time:	2005-264T00:00:07.500	Stop Time:	2005-264T23:59:59.948
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005265_01

Start Time:	2005-265T00:00:07.448	Stop Time:	2005-265T23:59:57.400
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005266_01

Start Time:	2005-266T00:00:08.646	Stop Time:	2005-266T23:59:58.594
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005267_01

Start Time:	2005-267T00:00:02.344	Stop Time:	2005-267T23:59:56.792
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005268_01

Start Time:	2005-268T00:00:08.042	Stop Time:	2005-268T23:59:57.240
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005269_01

Start Time:	2005-269T00:00:08.490	Stop Time:	2005-269T23:59:58.188
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005270_01

Start Time:	2005-270T00:00:20.688	Stop Time:	2005-270T23:59:57.636
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005271_01

Start Time:	2005-271T00:00:08.886	Stop Time:	2005-271T23:59:58.084
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005272_01

Start Time:	2005-272T00:00:09.334	Stop Time:	2005-272T23:59:56.204
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005273_01

Start Time:	2005-273T00:00:08.872	Stop Time:	2005-273T23:59:58.480
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005274_01

Start Time:	2005-274T00:00:09.730	Stop Time:	2005-274T23:59:58.928
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005275_01

Start Time:	2005-275T00:00:10.178	Stop Time:	2005-275T23:59:59.376
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005276_01

Start Time:	2005-276T00:00:05.001	Stop Time:	2005-276T23:59:57.824
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005277_01

Start Time:	2005-277T00:00:09.074	Stop Time:	2005-277T23:59:52.772
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005278_01

Start Time:	2005-278T00:00:04.022	Stop Time:	2005-278T23:59:50.470
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005279_01

Start Time:	2005-279T00:00:01.720	Stop Time:	2005-279T23:59:58.168
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005280_01

Start Time:	2005-280T00:00:05.668	Stop Time:	2005-280T23:59:57.616
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005281_01

Start Time:	2005-281T00:00:01.366	Stop Time:	2005-281T23:59:58.189
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005282_01

Start Time:	2005-282T00:00:01.314	Stop Time:	2005-282T23:59:55.012
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005283_01

Start Time:	2005-283T00:00:02.512	Stop Time:	2005-283T23:59:42.960
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005284_01

Start Time:	2005-284T00:00:05.464	Stop Time:	2005-284T23:59:59.408
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005285_01

Start Time:	2005-285T00:00:03.158	Stop Time:	2005-285T23:59:51.356
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005286_01

Start Time:	2005-286T00:00:02.606	Stop Time:	2005-286T23:59:56.304
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005287_01

Start Time:	2005-287T00:00:03.808	Stop Time:	2005-287T23:59:59.252
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005288_01

Start Time:	2005-288T00:00:06.752	Stop Time:	2005-288T23:59:55.700
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005289_01

Start Time:	2005-289T00:00:03.200	Stop Time:	2005-289T23:59:56.898
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005290_01

Start Time:	2005-290T00:00:00.648	Stop Time:	2005-290T23:59:54.600
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005291_01

Start Time:	2005-291T00:00:09.596	Stop Time:	2005-291T23:59:45.415
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005292_01

Start Time:	2005-292T00:00:07.786	Stop Time:	2005-292T23:59:58.242
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005293_01

Start Time:	2005-293T00:00:01.992	Stop Time:	2005-293T23:59:55.491
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005294_01

Start Time:	2005-294T00:00:01.799	Stop Time:	2005-294T23:59:50.388
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005295_01

Start Time:	2005-295T00:00:05.388	Stop Time:	2005-295T23:59:56.586
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005296_01

Start Time:	2005-296T00:00:00.336	Stop Time:	2005-296T23:59:54.284
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005297_01

Start Time:	2005-297T00:00:01.784	Stop Time:	2005-297T23:59:59.482
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005298_01

Start Time:	2005-298T00:00:03.232	Stop Time:	2005-298T23:59:57.180
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005299_01

Start Time:	2005-299T00:00:00.305	Stop Time:	2005-299T23:59:57.128
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005300_01

Start Time:	2005-300T00:00:00.878	Stop Time:	2005-300T23:59:58.576
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005301_01

Start Time:	2005-301T00:00:09.826	Stop Time:	2005-301T23:59:59.024
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005302_01

Start Time:	2005-302T00:00:10.274	Stop Time:	2005-302T23:59:58.347
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005303_01

Start Time:	2005-303T00:00:01.472	Stop Time:	2005-303T23:59:53.919
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005304_01

Start Time:	2005-304T00:00:05.169	Stop Time:	2005-304T23:59:57.367
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005305_01

Start Time:	2005-305T00:00:01.117	Stop Time:	2005-305T23:59:59.065
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005306_01

Start Time:	2005-306T00:00:02.815	Stop Time:	2005-306T23:59:56.763
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005307_01

Start Time:	2005-307T00:00:00.513	Stop Time:	2005-307T23:59:53.801
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005308_01

Start Time:	2005-308T00:00:00.094	Stop Time:	2005-308T23:59:59.909
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005309_01

Start Time:	2005-309T00:00:03.659	Stop Time:	2005-309T23:59:49.412
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005310_01

Start Time:	2005-310T00:00:14.712	Stop Time:	2005-310T23:59:47.559
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005311_01

Start Time:	2005-311T00:00:10.055	Stop Time:	2005-311T23:59:56.503
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005312_01

Start Time:	2005-312T00:00:04.003	Stop Time:	2005-312T23:59:55.451
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005313_01

Start Time:	2005-313T00:00:02.951	Stop Time:	2005-313T23:59:57.899
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005314_01

Start Time:	2005-314T00:00:01.024	Stop Time:	2005-314T23:59:57.222
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005315_01

Start Time:	2005-315T00:00:00.347	Stop Time:	2005-315T23:59:58.045
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005316_01

Start Time:	2005-316T00:00:01.795	Stop Time:	2005-316T23:59:57.993
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005317_01

Start Time:	2005-317T00:00:01.118	Stop Time:	2005-317T23:59:59.441
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005318_01

Start Time:	2005-318T00:00:03.191	Stop Time:	2005-318T23:59:59.639
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005319_01

Start Time:	2005-319T00:00:02.764	Stop Time:	2005-319T23:59:58.962
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005320_01

Start Time:	2005-320T00:00:02.087	Stop Time:	2005-320T23:59:57.285
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005321_01

Start Time:	2005-321T00:00:08.535	Stop Time:	2005-321T23:59:51.487
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005322_01

Start Time:	2005-322T00:00:00.858	Stop Time:	2005-322T23:59:53.556
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005323_01

Start Time:	2005-323T00:00:02.935	Stop Time:	2005-323T23:59:59.129
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005324_01

Start Time:	2005-324T00:00:02.879	Stop Time:	2005-324T23:59:58.077
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005325_01

Start Time:	2005-325T00:00:07.452	Stop Time:	2005-325T23:59:57.025
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005326_01

Start Time:	2005-326T00:00:00.775	Stop Time:	2005-326T23:59:59.098
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005327_01

Start Time:	2005-327T00:00:02.223	Stop Time:	2005-327T23:59:54.511
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005328_01

Start Time:	2005-328T00:00:00.843	Stop Time:	2005-328T23:59:57.244
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005329_01

Start Time:	2005-329T00:00:00.369	Stop Time:	2005-329T23:59:53.067
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005330_01

Start Time:	2005-330T00:00:04.317	Stop Time:	2005-330T23:59:53.515
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005331_01

Start Time:	2005-331T00:00:04.765	Stop Time:	2005-331T23:59:56.600
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005332_01

Start Time:	2005-332T00:00:09.237	Stop Time:	2005-332T23:59:59.036
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005333_01

Start Time:	2005-333T00:00:02.161	Stop Time:	2005-333T23:59:55.863
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005334_01

Start Time:	2005-334T00:00:07.109	Stop Time:	2005-334T23:59:56.311
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005335_01

Start Time:	2005-335T00:00:07.557	Stop Time:	2005-335T23:59:58.005
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005336_01

Start Time:	2005-336T00:00:01.130	Stop Time:	2005-336T23:59:59.313
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005337_01

Start Time:	2005-337T00:00:24.422	Stop Time:	2005-337T23:59:57.901
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005338_01

Start Time:	2005-338T00:00:01.026	Stop Time:	2005-338T23:59:56.349
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005339_01

Start Time:	2005-339T00:00:07.599	Stop Time:	2005-339T23:59:59.797
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005340_01

Start Time:	2005-340T00:00:11.047	Stop Time:	2005-340T23:59:56.999
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005341_01

Start Time:	2005-341T00:00:09.616	Stop Time:	2005-341T23:59:59.447
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005342_01

Start Time:	2005-342T00:00:21.943	Stop Time:	2005-342T23:59:57.891
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005343_01

Start Time:	2005-343T00:00:01.016	Stop Time:	2005-343T23:59:58.839
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005344_01

Start Time:	2005-344T00:00:10.089	Stop Time:	2005-344T23:59:59.538
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005345_01

Start Time:	2005-345T00:00:08.912	Stop Time:	2005-345T23:59:52.974
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005346_01

Start Time:	2005-346T00:00:05.657	Stop Time:	2005-346T23:59:59.809
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005347_01

Start Time:	2005-347T00:00:02.934	Stop Time:	2005-347T23:59:53.772
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005348_01

Start Time:	2005-348T00:00:00.065	Stop Time:	2005-348T23:59:58.580
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005349_01

Start Time:	2005-349T00:00:01.705	Stop Time:	2005-349T23:59:59.536
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005350_01

Start Time:	2005-350T00:00:05.794	Stop Time:	2005-350T23:59:58.037
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005351_01

Start Time:	2005-351T00:00:01.162	Stop Time:	2005-351T23:59:57.209
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005352_01

Start Time:	2005-352T00:00:03.560	Stop Time:	2005-352T23:59:59.928
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005353_01

Start Time:	2005-353T00:00:03.053	Stop Time:	2005-353T23:59:58.273
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005354_01

Start Time:	2005-354T00:00:04.503	Stop Time:	2005-354T23:59:56.445
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005355_01

Start Time:	2005-355T00:00:00.195	Stop Time:	2005-355T23:59:57.891
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005356_01

Start Time:	2005-356T00:00:01.641	Stop Time:	2005-356T23:59:56.537
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005357_01

Start Time:	2005-357T00:00:02.876	Stop Time:	2005-357T23:59:59.283
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005358_01

Start Time:	2005-358T00:00:02.408	Stop Time:	2005-358T23:59:59.604
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005359_01

Start Time:	2005-359T00:00:02.729	Stop Time:	2005-359T23:59:37.515
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005360_01

Start Time:	2005-360T00:00:02.562	Stop Time:	2005-360T23:59:59.621
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005361_01

Start Time:	2005-361T00:00:02.746	Stop Time:	2005-361T23:59:57.817
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005362_01

Start Time:	2005-362T00:00:05.321	Stop Time:	2005-362T23:59:55.763
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005363_01

Start Time:	2005-363T00:00:03.263	Stop Time:	2005-363T23:59:52.959
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005364_01

Start Time:	2005-364T00:00:02.334	Stop Time:	2005-364T23:59:57.155
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

LPHAFULL0_2005365_01

Start Time:	2005-365T00:00:08.405	Stop Time:	2005-365T23:59:57.602
The data columns contain full time resolution of LEMMS PHA data. The fill value for data in this file is -1.0E38. These data are background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. The background levels change over time and each channel's background level as a function of time in counts/sec is listed in the MIMI calibration file (described in the MIMI Data User Guide, the SIS for this dataset, and also in SIS for the uncalibrated MIMI data). There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. The MIMI instrument paper describes these channels, as does the MIMI Data User Guide. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). Note that a subset of the available PHA channels are typically used for science analysis, and only these channels are plotted here. The dataset catalog file details the reasons for this. Essentially, the efficiencies are unknown or uncertain for omitted channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angle of the LET.

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