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Cassini >> MIMI

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

Start Time: 2004-01-01 08:00:00 - Stop Time: 2017-09-17 07:00:00

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

Citiation Information

Author	Vandegriff J., Kusterer M.B.
Title	CASSINI SATURN MIMI CHEMS CALIBRATED DATA ARCHIVE
Publisher	NASA Planetary Data System
Publication Year	2018
doi	https://doi.org/10.17189/1519606

Top/ DATA/ CMFULL0/ 2013 /

CMFULL0_2013001_01

Start Time:	2013-001T00:01:06.653	Stop Time:	2013-001T23:54:37.106
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013002_01

Start Time:	2013-002T00:00:29.104	Stop Time:	2013-002T23:59:52.556
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013003_01

Start Time:	2013-003T00:05:44.553	Stop Time:	2013-003T23:59:19.023
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013004_01

Start Time:	2013-004T00:01:19.022	Stop Time:	2013-004T23:57:18.600
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013005_01

Start Time:	2013-005T00:00:18.599	Stop Time:	2013-005T23:58:49.051
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013006_01

Start Time:	2013-006T00:01:49.049	Stop Time:	2013-006T23:58:48.502
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013007_01

Start Time:	2013-007T00:01:48.501	Stop Time:	2013-007T23:57:03.954
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013008_01

Start Time:	2013-008T00:00:03.953	Stop Time:	2013-008T23:57:03.405
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013009_01

Start Time:	2013-009T00:00:03.404	Stop Time:	2013-009T23:59:19.856
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013010_01

Start Time:	2013-010T00:02:19.854	Stop Time:	2013-010T23:59:20.307
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013011_01

Start Time:	2013-011T00:02:19.306	Stop Time:	2013-011T23:57:47.759
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013012_01

Start Time:	2013-012T00:00:47.758	Stop Time:	2013-012T23:57:47.210
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013013_01

Start Time:	2013-013T00:00:47.209	Stop Time:	2013-013T23:57:47.661
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013014_01

Start Time:	2013-014T00:00:47.660	Stop Time:	2013-014T23:57:48.113
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013015_01

Start Time:	2013-015T00:00:48.111	Stop Time:	2013-015T23:54:31.425
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013016_01

Start Time:	2013-016T00:00:23.422	Stop Time:	2013-016T23:59:46.874
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013017_01

Start Time:	2013-017T00:05:38.872	Stop Time:	2013-017T23:59:09.325
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013018_01

Start Time:	2013-018T00:05:02.323	Stop Time:	2013-018T23:58:32.777
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013019_01

Start Time:	2013-019T00:04:24.775	Stop Time:	2013-019T23:59:56.368
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013020_01

Start Time:	2013-020T00:02:56.367	Stop Time:	2013-020T23:59:55.819
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013021_01

Start Time:	2013-021T00:02:55.817	Stop Time:	2013-021T23:59:14.270
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013022_01

Start Time:	2013-022T00:02:14.269	Stop Time:	2013-022T23:58:42.722
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013023_01

Start Time:	2013-023T00:01:42.720	Stop Time:	2013-023T23:58:42.173
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013024_01

Start Time:	2013-024T00:01:42.172	Stop Time:	2013-024T23:57:12.625
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013025_01

Start Time:	2013-025T00:00:12.624	Stop Time:	2013-025T23:57:13.076
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013026_01

Start Time:	2013-026T00:00:13.075	Stop Time:	2013-026T23:58:42.527
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013027_01

Start Time:	2013-027T00:01:42.526	Stop Time:	2013-027T23:58:57.978
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013028_01

Start Time:	2013-028T00:01:57.977	Stop Time:	2013-028T23:58:13.429
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013029_01

Start Time:	2013-029T00:01:13.428	Stop Time:	2013-029T23:59:20.755
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013030_01

Start Time:	2013-030T00:01:20.755	Stop Time:	2013-030T23:58:55.332
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013031_01

Start Time:	2013-031T00:01:55.331	Stop Time:	2013-031T23:58:27.658
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013032_01

Start Time:	2013-032T00:00:27.657	Stop Time:	2013-032T23:57:25.235
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013033_01

Start Time:	2013-033T00:00:25.234	Stop Time:	2013-033T23:59:54.685
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013034_01

Start Time:	2013-034T00:02:54.684	Stop Time:	2013-034T23:57:54.137
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013035_01

Start Time:	2013-035T00:00:54.136	Stop Time:	2013-035T23:57:53.589
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013036_01

Start Time:	2013-036T00:00:53.587	Stop Time:	2013-036T23:57:54.040
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013037_01

Start Time:	2013-037T00:00:54.039	Stop Time:	2013-037T23:57:54.491
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013038_01

Start Time:	2013-038T00:00:54.490	Stop Time:	2013-038T23:57:54.006
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013039_01

Start Time:	2013-039T00:00:54.005	Stop Time:	2013-039T23:57:54.457
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013040_01

Start Time:	2013-040T00:00:54.455	Stop Time:	2013-040T23:57:54.907
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013041_01

Start Time:	2013-041T00:00:54.906	Stop Time:	2013-041T23:57:54.358
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013042_01

Start Time:	2013-042T00:00:54.356	Stop Time:	2013-042T23:57:54.808
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013043_01

Start Time:	2013-043T00:00:54.807	Stop Time:	2013-043T23:57:31.118
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013044_01

Start Time:	2013-044T00:03:23.116	Stop Time:	2013-044T23:56:53.569
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013045_01

Start Time:	2013-045T00:02:46.567	Stop Time:	2013-045T23:57:00.160
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013046_01

Start Time:	2013-046T00:00:00.159	Stop Time:	2013-046T23:59:59.609
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013047_01

Start Time:	2013-047T00:02:59.608	Stop Time:	2013-047T23:59:15.998
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013048_01

Start Time:	2013-048T00:01:45.997	Stop Time:	2013-048T23:59:00.511
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013049_01

Start Time:	2013-049T00:02:00.510	Stop Time:	2013-049T23:59:00.961
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013050_01

Start Time:	2013-050T00:02:00.960	Stop Time:	2013-050T23:58:47.412
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013051_01

Start Time:	2013-051T00:01:47.411	Stop Time:	2013-051T23:55:55.801
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013052_01

Start Time:	2013-052T00:00:11.194	Stop Time:	2013-052T23:59:22.313
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013053_01

Start Time:	2013-053T00:02:22.312	Stop Time:	2013-053T23:59:28.763
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013054_01

Start Time:	2013-054T00:02:28.762	Stop Time:	2013-054T23:58:21.089
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013055_01

Start Time:	2013-055T00:00:21.088	Stop Time:	2013-055T23:57:43.997
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013056_01

Start Time:	2013-056T00:02:00.210	Stop Time:	2013-056T23:59:01.990
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013057_01

Start Time:	2013-057T00:01:01.989	Stop Time:	2013-057T23:57:30.566
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013058_01

Start Time:	2013-058T00:00:30.565	Stop Time:	2013-058T23:57:31.016
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013059_01

Start Time:	2013-059T00:00:31.015	Stop Time:	2013-059T23:57:30.467
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013060_01

Start Time:	2013-060T00:00:31.466	Stop Time:	2013-060T23:57:30.917
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013061_01

Start Time:	2013-061T00:00:30.916	Stop Time:	2013-061T23:57:31.368
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013062_01

Start Time:	2013-062T00:00:31.367	Stop Time:	2013-062T23:57:31.818
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013063_01

Start Time:	2013-063T00:00:31.817	Stop Time:	2013-063T23:57:31.269
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013064_01

Start Time:	2013-064T00:00:31.268	Stop Time:	2013-064T23:57:31.719
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013065_01

Start Time:	2013-065T00:00:31.718	Stop Time:	2013-065T23:57:31.170
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013066_01

Start Time:	2013-066T00:00:31.169	Stop Time:	2013-066T23:57:31.620
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013067_01

Start Time:	2013-067T00:00:31.619	Stop Time:	2013-067T23:57:32.071
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013068_01

Start Time:	2013-068T00:00:32.070	Stop Time:	2013-068T23:58:17.520
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013069_01

Start Time:	2013-069T00:01:17.519	Stop Time:	2013-069T23:58:17.971
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013070_01

Start Time:	2013-070T00:01:17.969	Stop Time:	2013-070T23:58:17.421
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013071_01

Start Time:	2013-071T00:01:17.420	Stop Time:	2013-071T23:59:42.801
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013072_01

Start Time:	2013-072T00:03:57.448	Stop Time:	2013-072T23:59:57.138
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013073_01

Start Time:	2013-073T00:04:12.476	Stop Time:	2013-073T23:57:09.773
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013074_01

Start Time:	2013-074T00:00:09.772	Stop Time:	2013-074T23:57:37.356
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013075_01

Start Time:	2013-075T00:01:52.608	Stop Time:	2013-075T23:56:59.639
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013076_01

Start Time:	2013-076T00:01:14.442	Stop Time:	2013-076T23:59:27.866
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013077_01

Start Time:	2013-077T00:03:43.474	Stop Time:	2013-077T23:58:55.574
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013078_01

Start Time:	2013-078T00:01:55.573	Stop Time:	2013-078T23:57:37.025
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013079_01

Start Time:	2013-079T00:00:37.024	Stop Time:	2013-079T23:59:42.475
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013080_01

Start Time:	2013-080T00:02:42.474	Stop Time:	2013-080T23:59:43.926
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013081_01

Start Time:	2013-081T00:02:43.924	Stop Time:	2013-081T23:59:52.376
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013082_01

Start Time:	2013-082T00:02:52.375	Stop Time:	2013-082T23:59:24.827
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013083_01

Start Time:	2013-083T00:02:24.826	Stop Time:	2013-083T23:58:50.277
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013084_01

Start Time:	2013-084T00:01:50.276	Stop Time:	2013-084T23:58:50.728
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013085_01

Start Time:	2013-085T00:01:50.727	Stop Time:	2013-085T23:59:23.053
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013086_01

Start Time:	2013-086T00:01:23.052	Stop Time:	2013-086T23:59:24.504
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013087_01

Start Time:	2013-087T00:01:24.503	Stop Time:	2013-087T23:58:29.954
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013088_01

Start Time:	2013-088T00:00:29.954	Stop Time:	2013-088T23:59:07.405
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013089_01

Start Time:	2013-089T00:01:07.404	Stop Time:	2013-089T23:58:23.856
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013090_01

Start Time:	2013-090T00:00:23.855	Stop Time:	2013-090T23:58:42.306
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013091_01

Start Time:	2013-091T00:00:42.305	Stop Time:	2013-091T23:59:43.756
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013092_01

Start Time:	2013-092T00:01:43.755	Stop Time:	2013-092T23:58:14.207
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013093_01

Start Time:	2013-093T00:00:14.206	Stop Time:	2013-093T23:57:12.783
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013094_01

Start Time:	2013-094T00:00:12.782	Stop Time:	2013-094T23:57:13.233
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013095_01

Start Time:	2013-095T00:00:13.232	Stop Time:	2013-095T23:57:13.684
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013096_01

Start Time:	2013-096T00:00:13.683	Stop Time:	2013-096T23:58:21.681
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013097_01

Start Time:	2013-097T00:02:36.097	Stop Time:	2013-097T23:57:53.714
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013098_01

Start Time:	2013-098T00:02:10.716	Stop Time:	2013-098T23:57:21.035
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013099_01

Start Time:	2013-099T00:00:21.034	Stop Time:	2013-099T23:57:21.486
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013100_01

Start Time:	2013-100T00:00:21.485	Stop Time:	2013-100T23:59:53.810
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013101_01

Start Time:	2013-101T00:01:53.810	Stop Time:	2013-101T23:58:24.261
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013102_01

Start Time:	2013-102T00:00:24.261	Stop Time:	2013-102T23:58:22.837
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013103_01

Start Time:	2013-103T00:01:22.836	Stop Time:	2013-103T23:58:34.287
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013104_01

Start Time:	2013-104T00:01:34.286	Stop Time:	2013-104T23:57:50.738
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013105_01

Start Time:	2013-105T00:00:50.737	Stop Time:	2013-105T23:57:50.189
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013106_01

Start Time:	2013-106T00:00:50.187	Stop Time:	2013-106T23:57:50.639
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013107_01

Start Time:	2013-107T00:00:50.638	Stop Time:	2013-107T23:59:53.964
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013108_01

Start Time:	2013-108T00:01:53.963	Stop Time:	2013-108T23:59:55.414
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013109_01

Start Time:	2013-109T00:01:55.413	Stop Time:	2013-109T23:59:23.990
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013110_01

Start Time:	2013-110T00:02:23.989	Stop Time:	2013-110T23:59:24.440
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013111_01

Start Time:	2013-111T00:02:24.439	Stop Time:	2013-111T23:57:24.892
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013112_01

Start Time:	2013-112T00:00:24.890	Stop Time:	2013-112T23:57:25.342
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013113_01

Start Time:	2013-113T00:00:25.341	Stop Time:	2013-113T23:59:34.792
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013114_01

Start Time:	2013-114T00:02:34.791	Stop Time:	2013-114T23:59:35.242
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013115_01

Start Time:	2013-115T00:02:35.241	Stop Time:	2013-115T23:59:35.693
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013116_01

Start Time:	2013-116T00:02:35.692	Stop Time:	2013-116T23:59:35.143
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013117_01

Start Time:	2013-117T00:02:35.142	Stop Time:	2013-117T23:59:58.468
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013118_01

Start Time:	2013-118T00:01:58.468	Stop Time:	2013-118T23:59:06.919
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013119_01

Start Time:	2013-119T00:01:06.919	Stop Time:	2013-119T23:58:17.371
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013120_01

Start Time:	2013-120T00:00:17.370	Stop Time:	2013-120T23:58:14.947
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013121_01

Start Time:	2013-121T00:01:14.945	Stop Time:	2013-121T23:59:15.397
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013122_01

Start Time:	2013-122T00:02:15.396	Stop Time:	2013-122T23:57:23.235
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013123_01

Start Time:	2013-123T00:01:40.979	Stop Time:	2013-123T23:58:43.298
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013124_01

Start Time:	2013-124T00:01:43.297	Stop Time:	2013-124T23:57:38.100
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013125_01

Start Time:	2013-125T00:01:53.685	Stop Time:	2013-125T23:57:47.199
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013126_01

Start Time:	2013-126T00:00:47.198	Stop Time:	2013-126T23:57:47.650
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013127_01

Start Time:	2013-127T00:00:47.648	Stop Time:	2013-127T23:57:48.100
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013128_01

Start Time:	2013-128T00:00:48.099	Stop Time:	2013-128T23:57:47.551
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013129_01

Start Time:	2013-129T00:00:47.549	Stop Time:	2013-129T23:57:48.001
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013130_01

Start Time:	2013-130T00:00:48.000	Stop Time:	2013-130T23:57:48.451
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013131_01

Start Time:	2013-131T00:00:48.450	Stop Time:	2013-131T23:57:48.902
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013132_01

Start Time:	2013-132T00:00:48.901	Stop Time:	2013-132T23:59:47.352
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013133_01

Start Time:	2013-133T00:02:47.351	Stop Time:	2013-133T23:57:49.740
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013134_01

Start Time:	2013-134T00:02:06.133	Stop Time:	2013-134T23:56:28.383
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013135_01

Start Time:	2013-135T00:00:44.584	Stop Time:	2013-135T23:56:24.447
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013136_01

Start Time:	2013-136T00:00:41.035	Stop Time:	2013-136T23:57:31.154
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013137_01

Start Time:	2013-137T00:00:31.153	Stop Time:	2013-137T23:57:43.605
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013138_01

Start Time:	2013-138T00:00:43.604	Stop Time:	2013-138T23:57:44.055
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013139_01

Start Time:	2013-139T00:00:44.054	Stop Time:	2013-139T23:57:19.506
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013140_01

Start Time:	2013-140T00:00:19.505	Stop Time:	2013-140T23:58:20.956
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013141_01

Start Time:	2013-141T00:01:20.955	Stop Time:	2013-141T23:58:21.406
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013142_01

Start Time:	2013-142T00:01:21.405	Stop Time:	2013-142T23:58:20.857
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013143_01

Start Time:	2013-143T00:01:20.856	Stop Time:	2013-143T23:54:50.168
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013144_01

Start Time:	2013-144T00:00:42.166	Stop Time:	2013-144T23:59:50.089
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013145_01

Start Time:	2013-145T00:04:05.693	Stop Time:	2013-145T23:58:13.208
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013146_01

Start Time:	2013-146T00:01:13.207	Stop Time:	2013-146T23:54:18.520
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013147_01

Start Time:	2013-147T00:00:11.517	Stop Time:	2013-147T23:59:33.968
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013148_01

Start Time:	2013-148T00:05:26.966	Stop Time:	2013-148T23:58:35.560
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013149_01

Start Time:	2013-149T00:01:35.558	Stop Time:	2013-149T23:59:07.885
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013150_01

Start Time:	2013-150T00:01:07.884	Stop Time:	2013-150T23:59:37.460
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013151_01

Start Time:	2013-151T00:02:37.459	Stop Time:	2013-151T23:59:37.911
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013152_01

Start Time:	2013-152T00:02:37.909	Stop Time:	2013-152T23:59:38.361
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013153_01

Start Time:	2013-153T00:02:38.360	Stop Time:	2013-153T23:56:21.672
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013154_01

Start Time:	2013-154T00:02:13.670	Stop Time:	2013-154T23:58:14.263
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013155_01

Start Time:	2013-155T00:01:14.261	Stop Time:	2013-155T23:57:37.713
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013156_01

Start Time:	2013-156T00:00:37.712	Stop Time:	2013-156T23:59:02.163
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013157_01

Start Time:	2013-157T00:02:02.162	Stop Time:	2013-157T23:59:01.676
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013158_01

Start Time:	2013-158T00:02:01.675	Stop Time:	2013-158T23:59:02.128
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013159_01

Start Time:	2013-159T00:02:02.126	Stop Time:	2013-159T23:59:22.579
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013160_01

Start Time:	2013-160T00:02:22.578	Stop Time:	2013-160T23:58:36.030
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013161_01

Start Time:	2013-161T00:01:36.029	Stop Time:	2013-161T23:57:14.482
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013162_01

Start Time:	2013-162T00:00:14.481	Stop Time:	2013-162T23:59:49.932
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013163_01

Start Time:	2013-163T00:02:49.931	Stop Time:	2013-163T23:57:50.384
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013164_01

Start Time:	2013-164T00:00:50.383	Stop Time:	2013-164T23:59:02.991
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013165_01

Start Time:	2013-165T00:03:19.564	Stop Time:	2013-165T23:57:59.287
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013166_01

Start Time:	2013-166T00:00:59.286	Stop Time:	2013-166T23:57:15.738
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013167_01

Start Time:	2013-167T00:00:15.737	Stop Time:	2013-167T23:57:16.190
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013168_01

Start Time:	2013-168T00:00:16.189	Stop Time:	2013-168T23:36:15.650
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013169_01

Start Time:	2013-169T04:30:17.534	Stop Time:	2013-169T23:57:16.093
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013170_01

Start Time:	2013-170T00:00:16.092	Stop Time:	2013-170T23:57:16.544
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013171_01

Start Time:	2013-171T00:00:16.543	Stop Time:	2013-171T23:57:15.995
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013172_01

Start Time:	2013-172T00:00:15.994	Stop Time:	2013-172T23:57:16.447
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013173_01

Start Time:	2013-173T00:00:16.446	Stop Time:	2013-173T23:58:18.773
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013174_01

Start Time:	2013-174T00:00:18.772	Stop Time:	2013-174T23:59:04.223
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013175_01

Start Time:	2013-175T00:01:04.223	Stop Time:	2013-175T23:58:47.800
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013176_01

Start Time:	2013-176T00:01:47.799	Stop Time:	2013-176T23:58:18.251
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013177_01

Start Time:	2013-177T00:01:18.250	Stop Time:	2013-177T23:57:51.472
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013178_01

Start Time:	2013-178T00:02:06.857	Stop Time:	2013-178T23:56:42.506
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013179_01

Start Time:	2013-179T00:00:57.504	Stop Time:	2013-179T23:59:27.605
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013180_01

Start Time:	2013-180T00:02:27.603	Stop Time:	2013-180T23:59:32.798
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013181_01

Start Time:	2013-181T00:03:48.796	Stop Time:	2013-181T23:58:27.507
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013182_01

Start Time:	2013-182T00:01:27.506	Stop Time:	2013-182T23:58:54.958
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013183_01

Start Time:	2013-183T00:01:54.957	Stop Time:	2013-183T23:58:54.410
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013184_01

Start Time:	2013-184T00:01:54.409	Stop Time:	2013-184T23:56:21.053
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013185_01

Start Time:	2013-185T00:00:38.192	Stop Time:	2013-185T23:58:48.312
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013186_01

Start Time:	2013-186T00:01:48.311	Stop Time:	2013-186T23:59:50.763
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013187_01

Start Time:	2013-187T00:02:50.762	Stop Time:	2013-187T23:57:20.215
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013188_01

Start Time:	2013-188T00:00:20.214	Stop Time:	2013-188T23:57:04.667
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013189_01

Start Time:	2013-189T00:00:04.665	Stop Time:	2013-189T23:57:05.118
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013190_01

Start Time:	2013-190T00:00:05.117	Stop Time:	2013-190T23:57:05.569
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013191_01

Start Time:	2013-191T00:00:05.568	Stop Time:	2013-191T23:59:51.019
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013192_01

Start Time:	2013-192T00:02:51.018	Stop Time:	2013-192T23:57:41.471
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013193_01

Start Time:	2013-193T00:00:41.470	Stop Time:	2013-193T23:59:04.922
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013194_01

Start Time:	2013-194T00:02:04.921	Stop Time:	2013-194T23:58:23.506
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013195_01

Start Time:	2013-195T00:02:03.372	Stop Time:	2013-195T23:56:35.372
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013196_01

Start Time:	2013-196T00:00:52.355	Stop Time:	2013-196T23:56:31.242
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013197_01

Start Time:	2013-197T00:00:46.822	Stop Time:	2013-197T23:59:05.274
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013198_01

Start Time:	2013-198T00:03:23.053	Stop Time:	2013-198T23:57:54.370
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013199_01

Start Time:	2013-199T00:02:09.919	Stop Time:	2013-199T23:59:48.196
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013200_01

Start Time:	2013-200T00:04:04.194	Stop Time:	2013-200T23:59:34.956
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013201_01

Start Time:	2013-201T00:01:34.955	Stop Time:	2013-201T23:58:25.407
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013202_01

Start Time:	2013-202T00:00:25.406	Stop Time:	2013-202T23:57:27.984
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013203_01

Start Time:	2013-203T00:00:27.983	Stop Time:	2013-203T23:59:18.434
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013204_01

Start Time:	2013-204T00:02:18.433	Stop Time:	2013-204T23:59:03.887
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013205_01

Start Time:	2013-205T00:02:03.886	Stop Time:	2013-205T23:59:04.338
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013206_01

Start Time:	2013-206T00:02:04.337	Stop Time:	2013-206T23:58:34.789
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013207_01

Start Time:	2013-207T00:01:34.788	Stop Time:	2013-207T23:59:20.240
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013208_01

Start Time:	2013-208T00:02:20.239	Stop Time:	2013-208T23:58:27.692
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013209_01

Start Time:	2013-209T00:01:27.691	Stop Time:	2013-209T23:57:06.144
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013210_01

Start Time:	2013-210T00:00:06.143	Stop Time:	2013-210T23:58:58.594
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013211_01

Start Time:	2013-211T00:01:58.593	Stop Time:	2013-211T23:58:36.046
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013212_01

Start Time:	2013-212T00:01:36.044	Stop Time:	2013-212T23:58:20.497
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013213_01

Start Time:	2013-213T00:01:20.496	Stop Time:	2013-213T23:58:19.948
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013214_01

Start Time:	2013-214T00:01:19.947	Stop Time:	2013-214T23:58:24.399
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013215_01

Start Time:	2013-215T00:01:24.398	Stop Time:	2013-215T23:58:24.851
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013216_01

Start Time:	2013-216T00:01:24.850	Stop Time:	2013-216T23:58:25.302
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013217_01

Start Time:	2013-217T00:01:25.301	Stop Time:	2013-217T23:57:56.753
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013218_01

Start Time:	2013-218T00:00:56.752	Stop Time:	2013-218T23:59:29.079
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013219_01

Start Time:	2013-219T00:01:29.078	Stop Time:	2013-219T23:57:59.656
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013220_01

Start Time:	2013-220T00:00:59.655	Stop Time:	2013-220T23:59:53.106
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013221_01

Start Time:	2013-221T00:02:53.105	Stop Time:	2013-221T23:59:52.558
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013222_01

Start Time:	2013-222T00:02:52.556	Stop Time:	2013-222T23:56:30.869
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013223_01

Start Time:	2013-223T00:02:23.867	Stop Time:	2013-223T23:55:54.321
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013224_01

Start Time:	2013-224T00:01:46.319	Stop Time:	2013-224T23:57:58.771
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013225_01

Start Time:	2013-225T00:03:50.769	Stop Time:	2013-225T23:57:21.223
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013226_01

Start Time:	2013-226T00:03:14.221	Stop Time:	2013-226T23:58:48.689
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013227_01

Start Time:	2013-227T00:00:48.688	Stop Time:	2013-227T23:59:58.140
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013228_01

Start Time:	2013-228T00:01:58.139	Stop Time:	2013-228T23:57:31.717
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013229_01

Start Time:	2013-229T00:00:31.716	Stop Time:	2013-229T23:57:31.168
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013230_01

Start Time:	2013-230T00:00:31.167	Stop Time:	2013-230T23:57:31.620
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013231_01

Start Time:	2013-231T00:00:31.619	Stop Time:	2013-231T23:57:31.071
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013232_01

Start Time:	2013-232T00:00:31.070	Stop Time:	2013-232T23:57:31.522
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013233_01

Start Time:	2013-233T00:00:31.521	Stop Time:	2013-233T23:57:31.973
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013234_01

Start Time:	2013-234T00:00:31.972	Stop Time:	2013-234T23:59:04.299
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013235_01

Start Time:	2013-235T00:01:04.298	Stop Time:	2013-235T23:59:05.750
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013236_01

Start Time:	2013-236T00:01:05.750	Stop Time:	2013-236T23:59:07.202
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013237_01

Start Time:	2013-237T00:01:07.201	Stop Time:	2013-237T23:59:08.653
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013238_01

Start Time:	2013-238T00:01:08.652	Stop Time:	2013-238T23:59:10.104
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013239_01

Start Time:	2013-239T00:01:10.103	Stop Time:	2013-239T23:59:12.555
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013240_01

Start Time:	2013-240T00:01:12.555	Stop Time:	2013-240T23:59:44.006
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013241_01

Start Time:	2013-241T00:01:44.006	Stop Time:	2013-241T23:59:42.583
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013242_01

Start Time:	2013-242T00:02:42.581	Stop Time:	2013-242T23:57:58.972
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013243_01

Start Time:	2013-243T00:00:28.971	Stop Time:	2013-243T23:56:41.064
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013244_01

Start Time:	2013-244T00:00:56.836	Stop Time:	2013-244T23:58:00.937
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013245_01

Start Time:	2013-245T00:01:00.936	Stop Time:	2013-245T23:57:27.388
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013246_01

Start Time:	2013-246T00:00:27.387	Stop Time:	2013-246T23:57:27.840
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013247_01

Start Time:	2013-247T00:00:27.839	Stop Time:	2013-247T23:57:39.291
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013248_01

Start Time:	2013-248T00:00:39.290	Stop Time:	2013-248T23:57:39.742
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013249_01

Start Time:	2013-249T00:00:39.741	Stop Time:	2013-249T23:59:53.193
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013250_01

Start Time:	2013-250T00:02:53.191	Stop Time:	2013-250T23:58:25.519
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013251_01

Start Time:	2013-251T00:00:25.519	Stop Time:	2013-251T23:58:26.971
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013252_01

Start Time:	2013-252T00:00:26.970	Stop Time:	2013-252T23:57:25.548
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013253_01

Start Time:	2013-253T00:00:25.547	Stop Time:	2013-253T23:57:36.999
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013254_01

Start Time:	2013-254T00:00:36.998	Stop Time:	2013-254T23:57:37.451
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013255_01

Start Time:	2013-255T00:00:37.450	Stop Time:	2013-255T23:56:27.840
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013256_01

Start Time:	2013-256T00:00:45.670	Stop Time:	2013-256T23:58:01.228
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013257_01

Start Time:	2013-257T00:00:01.227	Stop Time:	2013-257T23:59:01.960
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013258_01

Start Time:	2013-258T00:03:17.767	Stop Time:	2013-258T23:57:11.643
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013259_01

Start Time:	2013-259T00:01:27.606	Stop Time:	2013-259T23:58:45.707
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013260_01

Start Time:	2013-260T00:01:45.705	Stop Time:	2013-260T23:58:45.158
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013261_01

Start Time:	2013-261T00:01:45.157	Stop Time:	2013-261T23:58:45.609
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013262_01

Start Time:	2013-262T00:01:45.608	Stop Time:	2013-262T23:59:18.935
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013263_01

Start Time:	2013-263T00:01:18.934	Stop Time:	2013-263T23:59:48.449
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013264_01

Start Time:	2013-264T00:02:18.448	Stop Time:	2013-264T23:59:05.838
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013265_01

Start Time:	2013-265T00:01:05.837	Stop Time:	2013-265T23:59:36.351
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013266_01

Start Time:	2013-266T00:02:06.350	Stop Time:	2013-266T23:59:04.865
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013267_01

Start Time:	2013-267T00:02:04.864	Stop Time:	2013-267T23:59:05.317
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013268_01

Start Time:	2013-268T00:02:05.315	Stop Time:	2013-268T23:59:05.768
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013269_01

Start Time:	2013-269T00:02:05.767	Stop Time:	2013-269T23:59:05.219
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013270_01

Start Time:	2013-270T00:02:05.218	Stop Time:	2013-270T23:59:35.670
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013271_01

Start Time:	2013-271T00:02:35.669	Stop Time:	2013-271T23:59:36.121
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013272_01

Start Time:	2013-272T00:02:36.120	Stop Time:	2013-272T23:55:57.578
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013273_01

Start Time:	2013-273T00:00:11.537	Stop Time:	2013-273T23:59:43.961
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013274_01

Start Time:	2013-274T00:03:59.960	Stop Time:	2013-274T23:58:45.351
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013275_01

Start Time:	2013-275T00:00:45.350	Stop Time:	2013-275T23:59:14.259
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013276_01

Start Time:	2013-276T00:03:28.081	Stop Time:	2013-276T23:57:31.379
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013277_01

Start Time:	2013-277T00:00:31.377	Stop Time:	2013-277T23:56:53.217
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013278_01

Start Time:	2013-278T00:01:08.375	Stop Time:	2013-278T23:58:21.281
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013279_01

Start Time:	2013-279T00:01:21.280	Stop Time:	2013-279T23:59:05.732
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013280_01

Start Time:	2013-280T00:02:05.731	Stop Time:	2013-280T23:59:47.183
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013281_01

Start Time:	2013-281T00:02:47.182	Stop Time:	2013-281T23:59:46.634
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013282_01

Start Time:	2013-282T00:02:46.633	Stop Time:	2013-282T23:59:47.085
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013283_01

Start Time:	2013-283T00:02:47.084	Stop Time:	2013-283T23:59:47.537
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013284_01

Start Time:	2013-284T00:02:47.535	Stop Time:	2013-284T23:59:46.988
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013285_01

Start Time:	2013-285T00:02:46.987	Stop Time:	2013-285T23:59:47.439
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013286_01

Start Time:	2013-286T00:02:47.438	Stop Time:	2013-286T23:59:19.766
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013287_01

Start Time:	2013-287T00:01:19.765	Stop Time:	2013-287T23:59:06.674
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013288_01

Start Time:	2013-288T00:03:21.110	Stop Time:	2013-288T23:59:57.793
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013289_01

Start Time:	2013-289T00:02:57.792	Stop Time:	2013-289T23:57:17.245
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013290_01

Start Time:	2013-290T00:00:17.244	Stop Time:	2013-290T23:59:50.695
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013291_01

Start Time:	2013-291T00:02:50.694	Stop Time:	2013-291T23:59:16.147
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013292_01

Start Time:	2013-292T00:02:16.146	Stop Time:	2013-292T23:59:16.598
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013293_01

Start Time:	2013-293T00:02:16.597	Stop Time:	2013-293T23:58:21.050
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013294_01

Start Time:	2013-294T00:00:52.924	Stop Time:	2013-294T23:59:51.501
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013295_01

Start Time:	2013-295T00:02:51.499	Stop Time:	2013-295T23:58:21.952
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013296_01

Start Time:	2013-296T00:01:21.951	Stop Time:	2013-296T23:58:22.404
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013297_01

Start Time:	2013-297T00:01:22.403	Stop Time:	2013-297T23:58:21.855
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013298_01

Start Time:	2013-298T00:01:21.854	Stop Time:	2013-298T23:58:22.306
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013299_01

Start Time:	2013-299T00:01:22.305	Stop Time:	2013-299T23:58:22.758
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013300_01

Start Time:	2013-300T00:01:22.756	Stop Time:	2013-300T23:58:22.209
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013301_01

Start Time:	2013-301T00:01:22.208	Stop Time:	2013-301T23:58:22.660
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013302_01

Start Time:	2013-302T00:01:22.659	Stop Time:	2013-302T23:58:23.111
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013303_01

Start Time:	2013-303T00:01:23.110	Stop Time:	2013-303T23:57:08.562
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013304_01

Start Time:	2013-304T00:00:08.561	Stop Time:	2013-304T23:57:08.013
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013305_01

Start Time:	2013-305T00:00:08.012	Stop Time:	2013-305T23:57:08.465
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013306_01

Start Time:	2013-306T00:00:08.464	Stop Time:	2013-306T23:57:08.916
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013307_01

Start Time:	2013-307T00:00:08.915	Stop Time:	2013-307T23:59:38.366
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013308_01

Start Time:	2013-308T00:02:38.365	Stop Time:	2013-308T23:59:38.818
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013309_01

Start Time:	2013-309T00:02:38.816	Stop Time:	2013-309T17:44:37.412
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013310_01

Start Time:	2013-310T13:26:39.961	Stop Time:	2013-310T23:59:38.720
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013311_01

Start Time:	2013-311T00:02:38.719	Stop Time:	2013-311T23:59:40.171
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013312_01

Start Time:	2013-312T00:02:40.170	Stop Time:	2013-312T23:59:38.623
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013313_01

Start Time:	2013-313T00:02:38.622	Stop Time:	2013-313T11:44:37.354
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013314_01

Start Time:	2013-314T09:02:39.867	Stop Time:	2013-314T23:59:37.525
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013315_01

Start Time:	2013-315T00:02:37.524	Stop Time:	2013-315T23:58:11.852
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013316_01

Start Time:	2013-316T00:00:11.851	Stop Time:	2013-316T23:59:40.428
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013317_01

Start Time:	2013-317T00:02:40.427	Stop Time:	2013-317T23:59:40.879
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013318_01

Start Time:	2013-318T00:02:40.878	Stop Time:	2013-318T23:59:41.330
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013319_01

Start Time:	2013-319T00:02:41.329	Stop Time:	2013-319T23:57:40.782
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013320_01

Start Time:	2013-320T00:00:40.781	Stop Time:	2013-320T23:57:41.234
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013321_01

Start Time:	2013-321T00:00:41.233	Stop Time:	2013-321T23:57:41.685
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013322_01

Start Time:	2013-322T00:00:41.684	Stop Time:	2013-322T23:57:55.136
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013323_01

Start Time:	2013-323T00:00:55.135	Stop Time:	2013-323T23:57:55.588
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013324_01

Start Time:	2013-324T00:00:55.586	Stop Time:	2013-324T23:58:16.039
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013325_01

Start Time:	2013-325T00:01:16.038	Stop Time:	2013-325T23:59:50.489
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013326_01

Start Time:	2013-326T00:02:50.488	Stop Time:	2013-326T23:59:58.941
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013327_01

Start Time:	2013-327T00:02:58.939	Stop Time:	2013-327T23:58:15.393
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013328_01

Start Time:	2013-328T00:01:15.391	Stop Time:	2013-328T23:57:24.844
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013329_01

Start Time:	2013-329T00:00:24.843	Stop Time:	2013-329T23:59:06.295
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013330_01

Start Time:	2013-330T00:02:06.294	Stop Time:	2013-330T23:58:45.746
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013331_01

Start Time:	2013-331T00:01:45.745	Stop Time:	2013-331T23:59:57.197
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013332_01

Start Time:	2013-332T00:02:57.196	Stop Time:	2013-332T23:56:38.036
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013333_01

Start Time:	2013-333T00:00:55.418	Stop Time:	2013-333T23:57:30.101
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013334_01

Start Time:	2013-334T00:00:30.099	Stop Time:	2013-334T23:58:48.364
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013335_01

Start Time:	2013-335T00:00:18.363	Stop Time:	2013-335T23:59:40.159
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013336_01

Start Time:	2013-336T00:03:53.579	Stop Time:	2013-336T23:58:36.454
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013337_01

Start Time:	2013-337T00:01:36.453	Stop Time:	2013-337T23:58:18.905
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013338_01

Start Time:	2013-338T00:01:18.904	Stop Time:	2013-338T23:59:47.356
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013339_01

Start Time:	2013-339T00:02:47.355	Stop Time:	2013-339T23:58:44.683
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013340_01

Start Time:	2013-340T00:00:44.682	Stop Time:	2013-340T23:59:15.134
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013341_01

Start Time:	2013-341T00:01:15.133	Stop Time:	2013-341T23:59:44.710
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013342_01

Start Time:	2013-342T00:02:44.709	Stop Time:	2013-342T23:59:44.161
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013343_01

Start Time:	2013-343T00:02:44.160	Stop Time:	2013-343T23:59:44.613
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013344_01

Start Time:	2013-344T00:02:44.612	Stop Time:	2013-344T23:59:45.064
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013345_01

Start Time:	2013-345T00:02:45.063	Stop Time:	2013-345T23:59:44.515
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013346_01

Start Time:	2013-346T00:02:44.514	Stop Time:	2013-346T23:59:44.967
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013347_01

Start Time:	2013-347T00:02:44.965	Stop Time:	2013-347T23:59:44.418
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013348_01

Start Time:	2013-348T00:02:44.417	Stop Time:	2013-348T23:59:44.869
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013349_01

Start Time:	2013-349T00:02:44.868	Stop Time:	2013-349T23:59:45.320
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013350_01

Start Time:	2013-350T00:02:45.319	Stop Time:	2013-350T23:59:44.772
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013351_01

Start Time:	2013-351T00:02:44.771	Stop Time:	2013-351T23:57:00.223
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013352_01

Start Time:	2013-352T00:00:00.222	Stop Time:	2013-352T23:56:00.640
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013353_01

Start Time:	2013-353T00:00:19.001	Stop Time:	2013-353T23:58:20.125
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013354_01

Start Time:	2013-354T00:01:20.124	Stop Time:	2013-354T23:58:29.576
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013355_01

Start Time:	2013-355T00:01:29.575	Stop Time:	2013-355T23:58:30.028
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013356_01

Start Time:	2013-356T00:01:30.027	Stop Time:	2013-356T23:58:30.479
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013357_01

Start Time:	2013-357T00:01:30.478	Stop Time:	2013-357T23:58:29.930
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013358_01

Start Time:	2013-358T00:01:29.929	Stop Time:	2013-358T23:58:30.382
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013359_01

Start Time:	2013-359T00:01:30.380	Stop Time:	2013-359T23:58:30.833
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013360_01

Start Time:	2013-360T00:01:30.832	Stop Time:	2013-360T23:58:30.284
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013361_01

Start Time:	2013-361T00:01:30.283	Stop Time:	2013-361T23:58:30.658
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013362_01

Start Time:	2013-362T00:01:30.657	Stop Time:	2013-362T23:56:53.039
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013363_01

Start Time:	2013-363T00:01:07.686	Stop Time:	2013-363T23:57:01.560
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013364_01

Start Time:	2013-364T00:00:01.559	Stop Time:	2013-364T23:57:03.558
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2013365_01

Start Time:	2013-365T00:01:19.974	Stop Time:	2013-365T23:58:55.524
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

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