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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/ 2014 /

CMFULL0_2014001_01

Start Time:	2014-001T00:02:25.523	Stop Time:	2014-001T23:58:59.787
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014002_01

Start Time:	2014-002T00:01:41.974	Stop Time:	2014-002T23:57:14.426
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014003_01

Start Time:	2014-003T00:00:44.425	Stop Time:	2014-003T23:59:30.814
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014004_01

Start Time:	2014-004T00:02:30.813	Stop Time:	2014-004T23:59:31.265
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014005_01

Start Time:	2014-005T00:02:31.264	Stop Time:	2014-005T23:59:30.716
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014006_01

Start Time:	2014-006T00:02:30.715	Stop Time:	2014-006T23:58:50.167
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014007_01

Start Time:	2014-007T00:01:50.166	Stop Time:	2014-007T23:57:06.775
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014008_01

Start Time:	2014-008T00:01:22.773	Stop Time:	2014-008T23:59:46.616
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014009_01

Start Time:	2014-009T00:03:59.837	Stop Time:	2014-009T23:55:54.873
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014010_01

Start Time:	2014-010T00:00:09.906	Stop Time:	2014-010T22:23:31.070
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014011_01

Start Time:	2014-011T12:04:36.569	Stop Time:	2014-011T23:58:36.297
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014012_01

Start Time:	2014-012T00:00:36.296	Stop Time:	2014-012T23:59:18.935
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_2014013_01

Start Time:	2014-013T00:02:48.934	Stop Time:	2014-013T23:59:38.198
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014014_01

Start Time:	2014-014T00:01:38.198	Stop Time:	2014-014T23:58:26.837
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_2014015_01

Start Time:	2014-015T00:01:56.836	Stop Time:	2014-015T23:56:58.289
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014016_01

Start Time:	2014-016T00:00:28.288	Stop Time:	2014-016T23:57:37.740
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_2014017_01

Start Time:	2014-017T00:01:07.738	Stop Time:	2014-017T23:59:40.190
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_2014018_01

Start Time:	2014-018T00:03:10.188	Stop Time:	2014-018T23:57:52.735
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014019_01

Start Time:	2014-019T00:01:45.640	Stop Time:	2014-019T23:56:47.093
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_2014020_01

Start Time:	2014-020T00:00:17.091	Stop Time:	2014-020T23:57:19.481
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014021_01

Start Time:	2014-021T00:00:19.480	Stop Time:	2014-021T23:57:18.931
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014022_01

Start Time:	2014-022T00:00:18.930	Stop Time:	2014-022T23:57:19.382
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_2014023_01

Start Time:	2014-023T00:00:19.381	Stop Time:	2014-023T23:57:19.833
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_2014024_01

Start Time:	2014-024T00:00:19.832	Stop Time:	2014-024T23:57:19.284
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_2014025_01

Start Time:	2014-025T00:00:19.283	Stop Time:	2014-025T23:57:19.735
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014026_01

Start Time:	2014-026T00:00:19.734	Stop Time:	2014-026T23:57:20.186
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014027_01

Start Time:	2014-027T00:00:20.185	Stop Time:	2014-027T23:57:12.637
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014028_01

Start Time:	2014-028T00:00:12.636	Stop Time:	2014-028T23:58:28.087
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014029_01

Start Time:	2014-029T00:01:28.086	Stop Time:	2014-029T23:58:35.538
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014030_01

Start Time:	2014-030T00:01:35.537	Stop Time:	2014-030T23:58:09.989
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014031_01

Start Time:	2014-031T00:01:09.988	Stop Time:	2014-031T23:59:57.439
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_2014032_01

Start Time:	2014-032T00:02:57.438	Stop Time:	2014-032T23:58:32.891
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014033_01

Start Time:	2014-033T00:01:32.890	Stop Time:	2014-033T23:59:33.341
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014034_01

Start Time:	2014-034T00:02:33.340	Stop Time:	2014-034T23:57:33.793
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_2014035_01

Start Time:	2014-035T00:00:33.792	Stop Time:	2014-035T23:59:34.306
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_2014036_01

Start Time:	2014-036T00:03:04.305	Stop Time:	2014-036T23:59:36.694
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014037_01

Start Time:	2014-037T00:02:36.693	Stop Time:	2014-037T23:58:09.021
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014038_01

Start Time:	2014-038T00:00:09.020	Stop Time:	2014-038T23:57:08.597
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014039_01

Start Time:	2014-039T00:00:08.596	Stop Time:	2014-039T23:57:09.048
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014040_01

Start Time:	2014-040T00:00:09.047	Stop Time:	2014-040T23:59:10.373
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014041_01

Start Time:	2014-041T00:01:10.372	Stop Time:	2014-041T23:59:41.824
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014042_01

Start Time:	2014-042T00:01:41.823	Stop Time:	2014-042T23:58:13.276
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014043_01

Start Time:	2014-043T00:00:13.275	Stop Time:	2014-043T23:59:10.851
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_2014044_01

Start Time:	2014-044T00:02:10.850	Stop Time:	2014-044T23:58:43.177
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014045_01

Start Time:	2014-045T00:00:43.176	Stop Time:	2014-045T23:59:11.753
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_2014046_01

Start Time:	2014-046T00:02:11.752	Stop Time:	2014-046T23:58:49.204
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014047_01

Start Time:	2014-047T00:01:49.203	Stop Time:	2014-047T23:57:49.655
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014048_01

Start Time:	2014-048T00:00:49.654	Stop Time:	2014-048T23:57:11.107
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014049_01

Start Time:	2014-049T00:00:11.105	Stop Time:	2014-049T23:59:49.556
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_2014050_01

Start Time:	2014-050T00:02:49.555	Stop Time:	2014-050T23:59:49.007
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014051_01

Start Time:	2014-051T00:02:49.006	Stop Time:	2014-051T23:57:15.459
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014052_01

Start Time:	2014-052T00:00:15.458	Stop Time:	2014-052T23:57:14.910
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014053_01

Start Time:	2014-053T00:00:14.909	Stop Time:	2014-053T23:59:13.360
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014054_01

Start Time:	2014-054T00:02:13.359	Stop Time:	2014-054T23:59:13.811
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014055_01

Start Time:	2014-055T00:02:13.810	Stop Time:	2014-055T23:58:11.263
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_2014056_01

Start Time:	2014-056T00:01:11.262	Stop Time:	2014-056T23:58:11.714
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_2014057_01

Start Time:	2014-057T00:01:11.713	Stop Time:	2014-057T23:58:11.165
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014058_01

Start Time:	2014-058T00:01:11.163	Stop Time:	2014-058T23:58:11.616
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014059_01

Start Time:	2014-059T00:01:11.614	Stop Time:	2014-059T23:58:12.067
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014060_01

Start Time:	2014-060T00:01:12.065	Stop Time:	2014-060T23:58:11.517
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014061_01

Start Time:	2014-061T00:01:11.516	Stop Time:	2014-061T23:57:17.969
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014062_01

Start Time:	2014-062T00:00:17.968	Stop Time:	2014-062T23:58:50.419
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014063_01

Start Time:	2014-063T00:01:50.418	Stop Time:	2014-063T23:58:12.870
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014064_01

Start Time:	2014-064T00:01:12.869	Stop Time:	2014-064T23:57:27.384
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_2014065_01

Start Time:	2014-065T00:00:57.383	Stop Time:	2014-065T23:59:59.771
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_2014066_01

Start Time:	2014-066T00:02:59.770	Stop Time:	2014-066T23:59:30.223
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_2014067_01

Start Time:	2014-067T00:02:30.221	Stop Time:	2014-067T23:59:02.549
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014068_01

Start Time:	2014-068T00:01:02.548	Stop Time:	2014-068T23:59:26.123
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014069_01

Start Time:	2014-069T00:02:26.122	Stop Time:	2014-069T23:58:33.637
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014070_01

Start Time:	2014-070T00:02:03.636	Stop Time:	2014-070T23:58:16.088
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014071_01

Start Time:	2014-071T00:01:46.087	Stop Time:	2014-071T23:56:47.540
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014072_01

Start Time:	2014-072T00:00:17.538	Stop Time:	2014-072T23:57:10.084
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014073_01

Start Time:	2014-073T00:01:25.083	Stop Time:	2014-073T23:57:55.535
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014074_01

Start Time:	2014-074T00:02:10.533	Stop Time:	2014-074T23:56:09.987
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014075_01

Start Time:	2014-075T00:00:24.985	Stop Time:	2014-075T23:56:55.437
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014076_01

Start Time:	2014-076T00:01:10.436	Stop Time:	2014-076T23:57:40.888
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014077_01

Start Time:	2014-077T00:01:55.886	Stop Time:	2014-077T23:58:26.338
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_2014078_01

Start Time:	2014-078T00:02:41.337	Stop Time:	2014-078T23:59:10.789
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_2014079_01

Start Time:	2014-079T00:03:25.788	Stop Time:	2014-079T23:59:56.240
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_2014080_01

Start Time:	2014-080T00:04:11.238	Stop Time:	2014-080T23:56:26.692
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_2014081_01

Start Time:	2014-081T00:00:41.690	Stop Time:	2014-081T23:57:12.143
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_2014082_01

Start Time:	2014-082T00:01:27.141	Stop Time:	2014-082T23:59:11.593
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014083_01

Start Time:	2014-083T00:03:26.591	Stop Time:	2014-083T23:59:57.043
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014084_01

Start Time:	2014-084T00:04:12.042	Stop Time:	2014-084T23:57:49.495
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014085_01

Start Time:	2014-085T00:02:04.494	Stop Time:	2014-085T23:58:34.946
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014086_01

Start Time:	2014-086T00:02:49.944	Stop Time:	2014-086T23:56:29.398
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014087_01

Start Time:	2014-087T00:00:44.396	Stop Time:	2014-087T23:57:14.848
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014088_01

Start Time:	2014-088T00:01:29.847	Stop Time:	2014-088T23:59:27.298
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_2014089_01

Start Time:	2014-089T00:03:42.297	Stop Time:	2014-089T23:56:20.750
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_2014090_01

Start Time:	2014-090T00:00:39.522	Stop Time:	2014-090T23:58:23.201
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014091_01

Start Time:	2014-091T00:02:38.199	Stop Time:	2014-091T23:56:35.652
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014092_01

Start Time:	2014-092T00:00:50.651	Stop Time:	2014-092T23:58:34.102
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014093_01

Start Time:	2014-093T00:02:49.101	Stop Time:	2014-093T23:56:39.554
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014094_01

Start Time:	2014-094T00:00:54.552	Stop Time:	2014-094T23:57:54.004
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014095_01

Start Time:	2014-095T00:02:09.003	Stop Time:	2014-095T23:59:45.455
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014096_01

Start Time:	2014-096T00:04:00.453	Stop Time:	2014-096T23:57:32.750
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_2014097_01

Start Time:	2014-097T00:00:32.749	Stop Time:	2014-097T23:58:35.076
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_2014098_01

Start Time:	2014-098T00:00:35.075	Stop Time:	2014-098T23:57:34.652
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014099_01

Start Time:	2014-099T00:00:34.651	Stop Time:	2014-099T23:58:06.978
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_2014100_01

Start Time:	2014-100T00:00:06.977	Stop Time:	2014-100T23:59:17.428
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_2014101_01

Start Time:	2014-101T00:01:17.427	Stop Time:	2014-101T23:59:11.004
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014102_01

Start Time:	2014-102T00:02:11.003	Stop Time:	2014-102T23:59:43.330
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_2014103_01

Start Time:	2014-103T00:01:43.329	Stop Time:	2014-103T23:59:44.781
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014104_01

Start Time:	2014-104T00:01:44.780	Stop Time:	2014-104T23:58:11.357
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014105_01

Start Time:	2014-105T00:01:11.356	Stop Time:	2014-105T23:58:11.808
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_2014106_01

Start Time:	2014-106T00:01:11.807	Stop Time:	2014-106T23:59:54.258
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014107_01

Start Time:	2014-107T00:02:54.257	Stop Time:	2014-107T23:59:54.709
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014108_01

Start Time:	2014-108T00:02:54.708	Stop Time:	2014-108T12:33:03.422
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014109_01

Start Time:	2014-109T01:03:06.136	Stop Time:	2014-109T23:57:04.612
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014110_01

Start Time:	2014-110T00:00:04.611	Stop Time:	2014-110T23:57:18.063
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014111_01

Start Time:	2014-111T00:00:18.062	Stop Time:	2014-111T23:57:40.514
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014112_01

Start Time:	2014-112T00:00:40.513	Stop Time:	2014-112T23:58:21.965
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014113_01

Start Time:	2014-113T00:01:21.963	Stop Time:	2014-113T23:58:58.415
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014114_01

Start Time:	2014-114T00:01:58.414	Stop Time:	2014-114T23:58:42.866
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_2014115_01

Start Time:	2014-115T00:01:42.865	Stop Time:	2014-115T23:58:04.317
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_2014116_01

Start Time:	2014-116T00:01:04.316	Stop Time:	2014-116T23:58:03.768
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_2014117_01

Start Time:	2014-117T00:01:03.767	Stop Time:	2014-117T23:58:33.219
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_2014118_01

Start Time:	2014-118T00:01:33.218	Stop Time:	2014-118T23:58:32.670
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_2014119_01

Start Time:	2014-119T00:01:32.669	Stop Time:	2014-119T23:58:53.122
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014120_01

Start Time:	2014-120T00:01:53.121	Stop Time:	2014-120T23:58:53.573
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014121_01

Start Time:	2014-121T00:01:53.571	Stop Time:	2014-121T23:58:58.023
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_2014122_01

Start Time:	2014-122T00:01:58.022	Stop Time:	2014-122T23:58:57.474
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014123_01

Start Time:	2014-123T00:01:57.473	Stop Time:	2014-123T23:58:57.925
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014124_01

Start Time:	2014-124T00:01:57.924	Stop Time:	2014-124T23:58:58.376
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_2014125_01

Start Time:	2014-125T00:01:58.375	Stop Time:	2014-125T23:58:57.827
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_2014126_01

Start Time:	2014-126T00:01:57.826	Stop Time:	2014-126T23:58:58.278
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014127_01

Start Time:	2014-127T00:01:58.277	Stop Time:	2014-127T11:13:57.021
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014129_01

Start Time:	2014-129T10:55:58.929	Stop Time:	2014-129T23:58:58.631
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014130_01

Start Time:	2014-130T00:01:58.630	Stop Time:	2014-130T23:58:58.082
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014131_01

Start Time:	2014-131T00:01:58.080	Stop Time:	2014-131T23:58:58.533
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014132_01

Start Time:	2014-132T00:01:58.531	Stop Time:	2014-132T23:58:58.983
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014133_01

Start Time:	2014-133T00:01:58.982	Stop Time:	2014-133T23:57:58.435
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014134_01

Start Time:	2014-134T00:00:58.434	Stop Time:	2014-134T23:57:58.886
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014135_01

Start Time:	2014-135T00:00:58.884	Stop Time:	2014-135T23:57:59.337
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014136_01

Start Time:	2014-136T00:00:59.335	Stop Time:	2014-136T23:58:29.787
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014137_01

Start Time:	2014-137T00:01:29.786	Stop Time:	2014-137T23:58:00.238
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014138_01

Start Time:	2014-138T00:01:00.237	Stop Time:	2014-138T23:57:59.689
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_2014139_01

Start Time:	2014-139T00:00:59.688	Stop Time:	2014-139T23:57:37.140
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_2014140_01

Start Time:	2014-140T00:00:37.139	Stop Time:	2014-140T23:59:10.466
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014141_01

Start Time:	2014-141T00:01:10.465	Stop Time:	2014-141T23:57:10.042
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014142_01

Start Time:	2014-142T00:00:10.041	Stop Time:	2014-142T23:59:46.492
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014143_01

Start Time:	2014-143T00:02:46.491	Stop Time:	2014-143T23:59:46.943
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014144_01

Start Time:	2014-144T00:02:46.942	Stop Time:	2014-144T23:59:46.394
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014145_01

Start Time:	2014-145T00:02:46.393	Stop Time:	2014-145T23:59:46.845
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014146_01

Start Time:	2014-146T00:02:46.844	Stop Time:	2014-146T23:59:47.296
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014147_01

Start Time:	2014-147T00:02:47.295	Stop Time:	2014-147T23:59:46.747
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014148_01

Start Time:	2014-148T00:02:46.746	Stop Time:	2014-148T23:59:47.198
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014149_01

Start Time:	2014-149T00:02:47.196	Stop Time:	2014-149T23:59:47.648
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014150_01

Start Time:	2014-150T00:02:47.647	Stop Time:	2014-150T23:59:47.099
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014151_01

Start Time:	2014-151T00:02:47.098	Stop Time:	2014-151T23:59:47.550
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014152_01

Start Time:	2014-152T00:02:47.549	Stop Time:	2014-152T23:59:48.001
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_2014153_01

Start Time:	2014-153T00:02:48.000	Stop Time:	2014-153T23:59:47.452
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014154_01

Start Time:	2014-154T00:02:47.451	Stop Time:	2014-154T23:59:47.903
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014155_01

Start Time:	2014-155T00:02:47.902	Stop Time:	2014-155T23:59:39.354
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_2014156_01

Start Time:	2014-156T00:02:39.353	Stop Time:	2014-156T23:59:39.805
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014157_01

Start Time:	2014-157T00:02:39.804	Stop Time:	2014-157T23:59:06.256
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014158_01

Start Time:	2014-158T00:02:06.255	Stop Time:	2014-158T23:59:05.707
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_2014159_01

Start Time:	2014-159T00:02:05.706	Stop Time:	2014-159T23:58:12.158
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_2014160_01

Start Time:	2014-160T00:01:12.157	Stop Time:	2014-160T23:58:12.609
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_2014161_01

Start Time:	2014-161T00:01:12.608	Stop Time:	2014-161T23:57:40.060
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014162_01

Start Time:	2014-162T00:00:40.059	Stop Time:	2014-162T23:57:40.511
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_2014163_01

Start Time:	2014-163T00:00:40.510	Stop Time:	2014-163T23:57:02.962
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014164_01

Start Time:	2014-164T00:00:02.961	Stop Time:	2014-164T23:59:43.412
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_2014165_01

Start Time:	2014-165T00:02:43.411	Stop Time:	2014-165T23:58:56.863
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014166_01

Start Time:	2014-166T00:01:56.862	Stop Time:	2014-166T23:58:56.314
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014167_01

Start Time:	2014-167T00:01:56.313	Stop Time:	2014-167T23:58:58.640
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_2014168_01

Start Time:	2014-168T00:00:58.639	Stop Time:	2014-168T23:58:57.217
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_2014169_01

Start Time:	2014-169T00:01:57.216	Stop Time:	2014-169T23:58:57.618
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014170_01

Start Time:	2014-170T00:01:57.617	Stop Time:	2014-170T23:59:29.944
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014171_01

Start Time:	2014-171T00:01:29.943	Stop Time:	2014-171T23:58:58.519
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_2014172_01

Start Time:	2014-172T00:01:58.518	Stop Time:	2014-172T23:58:28.970
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014173_01

Start Time:	2014-173T00:01:28.969	Stop Time:	2014-173T23:58:29.420
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014174_01

Start Time:	2014-174T00:01:29.419	Stop Time:	2014-174T23:58:28.870
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014175_01

Start Time:	2014-175T00:01:28.869	Stop Time:	2014-175T23:58:29.321
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_2014176_01

Start Time:	2014-176T00:01:29.320	Stop Time:	2014-176T23:58:28.771
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_2014177_01

Start Time:	2014-177T00:01:28.770	Stop Time:	2014-177T23:58:29.222
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014178_01

Start Time:	2014-178T00:01:29.220	Stop Time:	2014-178T23:58:29.672
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_2014179_01

Start Time:	2014-179T00:01:29.671	Stop Time:	2014-179T23:59:42.700
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014180_01

Start Time:	2014-180T00:03:59.667	Stop Time:	2014-180T23:58:42.573
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014181_01

Start Time:	2014-181T00:01:42.571	Stop Time:	2014-181T23:56:47.766
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_2014182_01

Start Time:	2014-182T00:01:02.600	Stop Time:	2014-182T23:59:03.606
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014183_01

Start Time:	2014-183T00:03:21.409	Stop Time:	2014-183T23:58:46.275
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014184_01

Start Time:	2014-184T00:03:01.309	Stop Time:	2014-184T23:58:35.921
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014185_01

Start Time:	2014-185T00:02:51.919	Stop Time:	2014-185T23:58:43.403
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014186_01

Start Time:	2014-186T00:02:59.760	Stop Time:	2014-186T23:56:53.006
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_2014187_01

Start Time:	2014-187T00:01:08.407	Stop Time:	2014-187T23:57:22.726
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014188_01

Start Time:	2014-188T00:00:22.725	Stop Time:	2014-188T23:59:22.175
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014189_01

Start Time:	2014-189T00:02:22.174	Stop Time:	2014-189T23:59:21.626
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014190_01

Start Time:	2014-190T00:02:21.625	Stop Time:	2014-190T23:59:22.076
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_2014191_01

Start Time:	2014-191T00:02:22.075	Stop Time:	2014-191T23:59:21.526
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014192_01

Start Time:	2014-192T00:02:21.525	Stop Time:	2014-192T23:59:21.977
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014193_01

Start Time:	2014-193T00:02:21.976	Stop Time:	2014-193T23:59:22.427
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014194_01

Start Time:	2014-194T00:02:22.426	Stop Time:	2014-194T23:58:39.878
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014195_01

Start Time:	2014-195T00:01:39.877	Stop Time:	2014-195T23:58:45.328
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014196_01

Start Time:	2014-196T00:01:45.327	Stop Time:	2014-196T23:58:45.779
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014197_01

Start Time:	2014-197T00:01:45.777	Stop Time:	2014-197T23:58:00.229
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014198_01

Start Time:	2014-198T00:01:00.228	Stop Time:	2014-198T23:58:00.555
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_2014199_01

Start Time:	2014-199T00:00:00.554	Stop Time:	2014-199T23:59:39.004
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014200_01

Start Time:	2014-200T00:01:39.004	Stop Time:	2014-200T23:57:36.581
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014201_01

Start Time:	2014-201T00:00:36.579	Stop Time:	2014-201T23:57:37.031
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014202_01

Start Time:	2014-202T00:00:37.030	Stop Time:	2014-202T23:57:37.481
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014203_01

Start Time:	2014-203T00:00:37.480	Stop Time:	2014-203T23:57:40.283
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014204_01

Start Time:	2014-204T00:01:55.672	Stop Time:	2014-204T23:59:46.382
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_2014205_01

Start Time:	2014-205T00:02:46.381	Stop Time:	2014-205T23:59:22.833
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_2014206_01

Start Time:	2014-206T00:02:22.832	Stop Time:	2014-206T23:59:23.283
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014207_01

Start Time:	2014-207T00:02:23.282	Stop Time:	2014-207T23:59:23.733
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014208_01

Start Time:	2014-208T00:02:23.732	Stop Time:	2014-208T23:59:23.184
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014209_01

Start Time:	2014-209T00:02:23.183	Stop Time:	2014-209T23:58:28.764
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014210_01

Start Time:	2014-210T00:02:44.985	Stop Time:	2014-210T23:58:18.085
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_2014211_01

Start Time:	2014-211T00:01:18.084	Stop Time:	2014-211T23:58:18.535
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014212_01

Start Time:	2014-212T00:01:18.534	Stop Time:	2014-212T23:58:18.986
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014213_01

Start Time:	2014-213T00:01:18.985	Stop Time:	2014-213T23:58:18.436
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014214_01

Start Time:	2014-214T00:01:18.435	Stop Time:	2014-214T23:58:18.887
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_2014215_01

Start Time:	2014-215T00:01:18.885	Stop Time:	2014-215T23:58:19.337
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014216_01

Start Time:	2014-216T00:01:19.336	Stop Time:	2014-216T23:58:18.787
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014217_01

Start Time:	2014-217T00:01:18.786	Stop Time:	2014-217T23:58:19.238
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014218_01

Start Time:	2014-218T00:01:19.237	Stop Time:	2014-218T23:58:19.688
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014219_01

Start Time:	2014-219T00:01:19.687	Stop Time:	2014-219T23:58:19.138
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_2014220_01

Start Time:	2014-220T00:01:19.137	Stop Time:	2014-220T23:58:19.589
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_2014221_01

Start Time:	2014-221T00:01:19.588	Stop Time:	2014-221T23:57:47.039
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_2014222_01

Start Time:	2014-222T00:00:47.038	Stop Time:	2014-222T23:57:46.490
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014223_01

Start Time:	2014-223T00:00:46.489	Stop Time:	2014-223T23:57:46.940
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014224_01

Start Time:	2014-224T00:00:46.939	Stop Time:	2014-224T23:55:55.548
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_2014225_01

Start Time:	2014-225T00:00:10.327	Stop Time:	2014-225T23:57:02.841
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014226_01

Start Time:	2014-226T00:00:02.840	Stop Time:	2014-226T23:57:03.292
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014227_01

Start Time:	2014-227T00:00:03.290	Stop Time:	2014-227T23:57:03.742
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_2014228_01

Start Time:	2014-228T00:00:03.741	Stop Time:	2014-228T23:59:05.192
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014229_01

Start Time:	2014-229T00:02:05.190	Stop Time:	2014-229T23:57:51.642
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014230_01

Start Time:	2014-230T00:00:51.641	Stop Time:	2014-230T23:57:52.093
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_2014231_01

Start Time:	2014-231T00:00:52.092	Stop Time:	2014-231T23:57:22.543
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014232_01

Start Time:	2014-232T00:00:22.542	Stop Time:	2014-232T23:57:20.150
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014233_01

Start Time:	2014-233T00:01:35.148	Stop Time:	2014-233T23:57:22.444
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014234_01

Start Time:	2014-234T00:00:22.443	Stop Time:	2014-234T23:58:59.050
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_2014235_01

Start Time:	2014-235T00:03:14.049	Stop Time:	2014-235T23:58:00.501
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_2014236_01

Start Time:	2014-236T00:02:15.499	Stop Time:	2014-236T23:59:13.951
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014237_01

Start Time:	2014-237T00:03:28.949	Stop Time:	2014-237T23:56:12.402
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014238_01

Start Time:	2014-238T00:00:27.401	Stop Time:	2014-238T23:57:28.852
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_2014239_01

Start Time:	2014-239T00:01:43.851	Stop Time:	2014-239T23:58:14.302
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_2014240_01

Start Time:	2014-240T00:02:29.301	Stop Time:	2014-240T23:58:59.752
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014241_01

Start Time:	2014-241T00:03:14.751	Stop Time:	2014-241T23:56:04.204
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014242_01

Start Time:	2014-242T00:00:19.202	Stop Time:	2014-242T23:56:49.654
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014243_01

Start Time:	2014-243T00:01:04.652	Stop Time:	2014-243T23:58:08.104
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_2014244_01

Start Time:	2014-244T00:02:23.102	Stop Time:	2014-244T23:59:10.554
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014245_01

Start Time:	2014-245T00:03:25.552	Stop Time:	2014-245T23:56:22.005
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014246_01

Start Time:	2014-246T00:00:37.004	Stop Time:	2014-246T23:57:07.456
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014247_01

Start Time:	2014-247T00:01:22.454	Stop Time:	2014-247T23:59:06.905
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_2014248_01

Start Time:	2014-248T00:03:21.904	Stop Time:	2014-248T23:56:26.357
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014249_01

Start Time:	2014-249T00:00:41.355	Stop Time:	2014-249T23:58:16.806
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014250_01

Start Time:	2014-250T00:02:31.805	Stop Time:	2014-250T23:59:35.256
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014251_01

Start Time:	2014-251T00:03:50.255	Stop Time:	2014-251T23:57:40.707
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_2014252_01

Start Time:	2014-252T00:01:55.706	Stop Time:	2014-252T23:59:37.353
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014253_01

Start Time:	2014-253T00:03:53.770	Stop Time:	2014-253T23:56:28.610
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014254_01

Start Time:	2014-254T00:00:43.608	Stop Time:	2014-254T22:54:14.670
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_2014255_01

Start Time:	2014-255T10:57:23.804	Stop Time:	2014-255T23:59:23.509
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014256_01

Start Time:	2014-256T00:03:38.508	Stop Time:	2014-256T23:56:47.351
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_2014257_01

Start Time:	2014-257T00:01:01.572	Stop Time:	2014-257T23:57:51.411
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014258_01

Start Time:	2014-258T00:02:06.409	Stop Time:	2014-258T23:59:57.091
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014259_01

Start Time:	2014-259T00:04:11.280	Stop Time:	2014-259T23:56:44.312
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_2014260_01

Start Time:	2014-260T00:00:59.310	Stop Time:	2014-260T23:58:35.761
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014261_01

Start Time:	2014-261T00:02:50.760	Stop Time:	2014-261T23:59:48.055
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_2014262_01

Start Time:	2014-262T00:02:48.054	Stop Time:	2014-262T23:59:17.506
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_2014263_01

Start Time:	2014-263T00:02:17.505	Stop Time:	2014-263T23:59:15.956
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_2014264_01

Start Time:	2014-264T00:02:15.955	Stop Time:	2014-264T23:59:15.407
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_2014265_01

Start Time:	2014-265T00:02:15.405	Stop Time:	2014-265T23:56:12.991
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_2014266_01

Start Time:	2014-266T00:00:29.587	Stop Time:	2014-266T23:57:14.308
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014267_01

Start Time:	2014-267T00:00:14.307	Stop Time:	2014-267T23:59:23.500
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014268_01

Start Time:	2014-268T00:03:39.143	Stop Time:	2014-268T23:56:47.541
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014269_01

Start Time:	2014-269T00:01:00.977	Stop Time:	2014-269T23:58:18.206
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014270_01

Start Time:	2014-270T00:02:33.790	Stop Time:	2014-270T23:59:34.109
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014271_01

Start Time:	2014-271T00:02:34.108	Stop Time:	2014-271T23:55:44.717
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_2014272_01

Start Time:	2014-272T00:00:01.524	Stop Time:	2014-272T23:58:27.010
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014273_01

Start Time:	2014-273T00:01:27.009	Stop Time:	2014-273T23:58:27.460
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_2014274_01

Start Time:	2014-274T00:01:27.459	Stop Time:	2014-274T23:58:55.102
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014275_01

Start Time:	2014-275T00:03:11.261	Stop Time:	2014-275T23:58:42.361
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_2014276_01

Start Time:	2014-276T00:01:42.360	Stop Time:	2014-276T23:56:11.750
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_2014277_01

Start Time:	2014-277T00:00:25.389	Stop Time:	2014-277T23:58:43.262
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014278_01

Start Time:	2014-278T00:01:43.261	Stop Time:	2014-278T23:58:43.712
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014279_01

Start Time:	2014-279T00:01:43.711	Stop Time:	2014-279T23:58:43.163
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_2014280_01

Start Time:	2014-280T00:01:43.162	Stop Time:	2014-280T23:58:43.613
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_2014281_01

Start Time:	2014-281T00:01:43.612	Stop Time:	2014-281T23:58:44.064
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_2014282_01

Start Time:	2014-282T00:01:44.062	Stop Time:	2014-282T23:58:43.514
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014283_01

Start Time:	2014-283T00:01:43.513	Stop Time:	2014-283T23:58:43.964
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_2014284_01

Start Time:	2014-284T00:01:43.963	Stop Time:	2014-284T23:58:44.415
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014285_01

Start Time:	2014-285T00:01:44.414	Stop Time:	2014-285T23:58:43.865
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_2014286_01

Start Time:	2014-286T00:01:43.864	Stop Time:	2014-286T23:58:41.316
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014287_01

Start Time:	2014-287T00:01:41.314	Stop Time:	2014-287T19:43:39.863
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014288_01

Start Time:	2014-288T11:25:41.504	Stop Time:	2014-288T23:57:47.217
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_2014289_01

Start Time:	2014-289T00:00:47.216	Stop Time:	2014-289T23:57:47.667
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_2014290_01

Start Time:	2014-290T00:00:47.666	Stop Time:	2014-290T23:58:39.180
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014291_01

Start Time:	2014-291T00:02:09.178	Stop Time:	2014-291T23:57:16.697
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014292_01

Start Time:	2014-292T00:01:33.723	Stop Time:	2014-292T23:57:36.983
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014293_01

Start Time:	2014-293T00:01:53.173	Stop Time:	2014-293T23:58:03.473
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014294_01

Start Time:	2014-294T00:02:18.045	Stop Time:	2014-294T23:56:11.271
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014295_01

Start Time:	2014-295T00:00:26.074	Stop Time:	2014-295T06:33:51.768
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_2014296_01

Start Time:	2014-296T01:33:23.333	Stop Time:	2014-296T23:57:22.820
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014297_01

Start Time:	2014-297T00:00:22.819	Stop Time:	2014-297T23:58:49.602
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014298_01

Start Time:	2014-298T00:03:06.800	Stop Time:	2014-298T23:57:56.268
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014299_01

Start Time:	2014-299T00:02:13.047	Stop Time:	2014-299T23:59:09.233
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_2014300_01

Start Time:	2014-300T00:02:39.232	Stop Time:	2014-300T23:58:23.778
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014301_01

Start Time:	2014-301T00:02:38.776	Stop Time:	2014-301T23:58:25.228
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_2014302_01

Start Time:	2014-302T00:02:40.227	Stop Time:	2014-302T00:19:39.220
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014303_01

Start Time:	2014-303T08:12:10.486	Stop Time:	2014-303T23:59:55.127
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014304_01

Start Time:	2014-304T00:04:10.126	Stop Time:	2014-304T23:56:25.579
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_2014305_01

Start Time:	2014-305T00:00:40.578	Stop Time:	2014-305T23:57:10.029
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014306_01

Start Time:	2014-306T00:01:25.028	Stop Time:	2014-306T06:19:39.883
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014307_01

Start Time:	2014-307T11:22:11.214	Stop Time:	2014-307T23:58:40.930
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_2014308_01

Start Time:	2014-308T00:02:55.928	Stop Time:	2014-308T23:56:28.381
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014309_01

Start Time:	2014-309T00:00:43.379	Stop Time:	2014-309T23:57:13.831
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014310_01

Start Time:	2014-310T00:01:28.829	Stop Time:	2014-310T23:58:36.281
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_2014311_01

Start Time:	2014-311T00:02:51.279	Stop Time:	2014-311T23:59:21.731
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014312_01

Start Time:	2014-312T00:03:36.729	Stop Time:	2014-312T23:57:25.182
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014313_01

Start Time:	2014-313T00:01:40.181	Stop Time:	2014-313T23:58:10.632
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014314_01

Start Time:	2014-314T00:02:25.631	Stop Time:	2014-314T23:59:35.668
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014315_01

Start Time:	2014-315T00:03:50.862	Stop Time:	2014-315T23:56:40.534
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014316_01

Start Time:	2014-316T00:00:55.532	Stop Time:	2014-316T23:58:18.159
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_2014317_01

Start Time:	2014-317T00:02:35.755	Stop Time:	2014-317T23:58:50.277
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_2014318_01

Start Time:	2014-318T00:01:50.276	Stop Time:	2014-318T23:58:50.728
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_2014319_01

Start Time:	2014-319T00:01:50.727	Stop Time:	2014-319T23:58:50.178
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014320_01

Start Time:	2014-320T00:01:50.177	Stop Time:	2014-320T23:58:50.629
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014321_01

Start Time:	2014-321T00:01:50.628	Stop Time:	2014-321T23:58:49.079
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_2014322_01

Start Time:	2014-322T00:01:50.078	Stop Time:	2014-322T23:58:50.530
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014323_01

Start Time:	2014-323T00:01:50.528	Stop Time:	2014-323T23:58:49.980
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014324_01

Start Time:	2014-324T00:01:49.979	Stop Time:	2014-324T23:58:50.430
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014325_01

Start Time:	2014-325T00:01:50.429	Stop Time:	2014-325T23:58:18.881
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014326_01

Start Time:	2014-326T00:01:18.880	Stop Time:	2014-326T23:57:51.332
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_2014327_01

Start Time:	2014-327T00:00:51.330	Stop Time:	2014-327T23:57:39.552
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014328_01

Start Time:	2014-328T00:01:52.359	Stop Time:	2014-328T23:57:02.233
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_2014329_01

Start Time:	2014-329T00:00:02.232	Stop Time:	2014-329T23:58:33.683
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_2014330_01

Start Time:	2014-330T00:01:33.682	Stop Time:	2014-330T23:58:52.133
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014331_01

Start Time:	2014-331T00:01:52.132	Stop Time:	2014-331T23:58:52.583
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_2014332_01

Start Time:	2014-332T00:01:52.582	Stop Time:	2014-332T23:59:32.034
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014333_01

Start Time:	2014-333T00:02:32.032	Stop Time:	2014-333T23:58:24.484
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014334_01

Start Time:	2014-334T00:01:24.483	Stop Time:	2014-334T23:59:48.934
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014335_01

Start Time:	2014-335T00:02:48.933	Stop Time:	2014-335T23:55:53.964
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_2014336_01

Start Time:	2014-336T00:00:09.931	Stop Time:	2014-336T23:58:19.836
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014337_01

Start Time:	2014-337T00:01:19.835	Stop Time:	2014-337T23:57:31.286
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014338_01

Start Time:	2014-338T00:00:31.285	Stop Time:	2014-338T23:58:23.737
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014339_01

Start Time:	2014-339T00:25:23.726	Stop Time:	2014-339T23:57:53.187
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014340_01

Start Time:	2014-340T00:00:53.186	Stop Time:	2014-340T23:59:35.637
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014341_01

Start Time:	2014-341T00:02:35.636	Stop Time:	2014-341T23:58:46.088
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014342_01

Start Time:	2014-342T00:01:45.087	Stop Time:	2014-342T23:58:23.538
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014343_01

Start Time:	2014-343T00:01:23.537	Stop Time:	2014-343T23:58:53.989
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014344_01

Start Time:	2014-344T00:01:53.987	Stop Time:	2014-344T23:59:10.376
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_2014345_01

Start Time:	2014-345T00:01:40.375	Stop Time:	2014-345T23:59:39.889
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014346_01

Start Time:	2014-346T00:02:39.888	Stop Time:	2014-346T23:59:39.340
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014347_01

Start Time:	2014-347T00:02:39.338	Stop Time:	2014-347T23:59:39.790
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014348_01

Start Time:	2014-348T00:02:39.789	Stop Time:	2014-348T23:58:16.397
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_2014349_01

Start Time:	2014-349T00:02:29.009	Stop Time:	2014-349T23:59:06.691
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014350_01

Start Time:	2014-350T00:02:06.690	Stop Time:	2014-350T23:59:07.141
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014351_01

Start Time:	2014-351T00:02:07.136	Stop Time:	2014-351T23:59:06.556
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_2014352_01

Start Time:	2014-352T00:02:06.555	Stop Time:	2014-352T23:59:07.006
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_2014353_01

Start Time:	2014-353T00:02:07.005	Stop Time:	2014-353T23:59:07.455
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014354_01

Start Time:	2014-354T00:02:07.454	Stop Time:	2014-354T23:59:06.905
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_2014355_01

Start Time:	2014-355T00:02:06.904	Stop Time:	2014-355T23:59:07.354
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_2014356_01

Start Time:	2014-356T00:02:07.353	Stop Time:	2014-356T23:59:07.804
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014357_01

Start Time:	2014-357T00:02:07.803	Stop Time:	2014-357T23:59:07.253
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014358_01

Start Time:	2014-358T00:02:07.252	Stop Time:	2014-358T23:59:07.703
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014359_01

Start Time:	2014-359T00:02:07.701	Stop Time:	2014-359T23:58:04.090
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014360_01

Start Time:	2014-360T00:02:19.284	Stop Time:	2014-360T23:57:44.149
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014361_01

Start Time:	2014-361T00:02:00.733	Stop Time:	2014-361T23:58:08.989
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014362_01

Start Time:	2014-362T00:02:25.780	Stop Time:	2014-362T23:59:34.047
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014363_01

Start Time:	2014-363T00:03:49.241	Stop Time:	2014-363T23:59:57.950
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2014364_01

Start Time:	2014-364T00:02:57.949	Stop Time:	2014-364T23:59:34.399
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_2014365_01

Start Time:	2014-365T00:02:34.398	Stop Time:	2014-365T23:55:53.788
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included 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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